How Gravitational Waves May Revolutionize Dark Matter Detection

Researchers have unveiled a groundbreaking method for determining if black hole mergers transpired within dense clouds of dark matter, paving the way for new insights into one of astronomy’s greatest enigmas.

The gravitational waves recorded by LIGO captured the final moments of two black holes merging into a larger, rotating black hole. Image credit: T. Pyle / LIGO.

Dark matter is an elusive, virtual substance that doesn’t interact with electromagnetic forces, making it invisible and difficult to detect directly.

This mysterious matter allows light, magnetic fields, and other energies to traverse without leaving any observable trace.

The existence of dark matter is inferred solely through its gravitational influence, observable in how gravity bends around galaxies.

Astronomers recognize that this bending indicates a gravitational field, an influencing force outside a galaxy’s own gravity, responsible for lensing phenomena.

Current estimates suggest that dark matter constitutes more than 85% of the universe’s matter, yet its true nature remains hotly debated.

One theory posits the existence of light scalar particles, significantly lighter than electrons, as a form of dark matter.

The researchers hypothesize that dark matter behaves as both a particle and a wave as it approaches a black hole.

When dark matter waves interact with a rapidly spinning black hole, energy may be transferred, amplifying these waves through a phenomenon known as superradiation.

This results in a dense swirling of dark matter reminiscent of cream stirred into butter.

At extreme densities, this light scalar dark matter could leave distinctive imprints on gravitational waves emitted from colliding black holes, although questions remain about the specific nature of that signature.

Would such a signature be detectable in gravitational waves traveling from merging black holes millions of light-years away?

To explore these questions, MIT physicist Jos Aurecoechea and collaborators developed a model predicting gravitational waveforms that would occur if two black holes collided within a dark matter-rich environment instead of a vacuum.

“We know dark matter permeates our universe; it simply must be dense enough for us to observe its effects,” Dr. Aurekoetsea noted.

“Black holes serve as a unique mechanism for increasing dark matter density, and we can investigate this by studying the gravitational waves they emit during merges.”

The research team analyzed signals captured in the initial three observations from LIGO-Virgo-KAGRA (LVK), a global network of observatories dedicated to detecting gravitational waves from black hole mergers and other celestial events.

Among the 28 prominent signals, 27 were identified as originating from black holes merging in a vacuum.

However, one signal, a pattern identified in GW 190728, exhibited indications of a potential dark matter signature.

It’s important to note that, as of now, dark matter has not been directly observed.

This innovative approach provides a promising means to scrutinize gravitational wave data for hints of dark matter, which could be subsequently validated through other methods.

“This statistical significance isn’t high enough to confirm dark matter detection, and further verification by independent teams is essential,” Dr. Orekoetsea cautioned.

“Notably, without models like ours, a black hole merger occurring in a dark matter context might be mistakenly classified as having occurred in a vacuum.”

“As the LVK continues to gather data over the coming years, we may uncover new insights into dark matter surrounding black holes,” said Dr. Soumen Roy from the Catholic University of Leuven and the Royal Observatory of Belgium.

“This is an exhilarating time to delve into new physics through gravitational wave analysis.”

Dr. Rodrigo Vicente of the University of Amsterdam remarked, “Harnessing black holes to search for dark matter represents a monumental leap in our capabilities.”

“We can explore dark matter phenomena on a much smaller scale than previously possible.”

For further details, refer to the findings published today in Physical Review Letters.

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Somen Roy et al. 2026. Scalar Field Around the LIGO-Virgo-KAGRA Black Hole Binary. Physics Review Letters 136, 191402; doi: 10.1103/fv9z-zkxx

Source: www.sci.news

Ancient 300-Year-Old Experiment Poised to Revolutionize Dark Matter Detection

Dark Matter: The Dominant Force in the Universe

Image processing by ESA/Euclid/Euclid Consortium/NASA; M. Schirmer (MPIA, Heidelberg)

Centuries of scientific experimentation are paving the way for a breakthrough in the hunt for new particles, particularly those believed to constitute dark matter.

In 1773, British scientist Henry Cavendish initiated an experiment aimed at unraveling the mysteries of electromagnetism, involving the measurement of electrical potential on two nested metal shells to examine interactions of charged particles.

Now, Peter Graham, a professor at Stanford University, suggests reviving Cavendish’s historic experiment could illuminate the enigmatic particles forming dark matter.

Dark matter, which constitutes a significant portion of our universe, remains poorly understood. Numerous theories have emerged regarding its composition, and experiments range from particle colliders to advanced underground detectors.

Graham and his research team are focusing on a dark matter candidate known as milli-charged particles (mCPs). True to its name, mCP has an exceptionally small charge, rendering it suitable for Cavendish’s original experimental setup.

The team proposes recreating the nested shell design, applying a voltage to the outer shell and measuring the voltage difference to detect the presence of mCPs during the experiment.

Exploring Electromagnetism: Henry Cavendish’s 18th Century Experiments

Cavendish Institute

To enhance the experimental design, the team plans to incorporate an accumulator device to effectively extract all charged particles from the surrounding environment, maximizing the potential for mCP detection, according to Harikrishnan Ramani of the University of Delaware.

This innovative design is cost-effective compared to other mCP explorations, estimated at under $1 million—1,000 times less than operating a particle accelerator for a year. Preliminary calculations indicate it could be more sensitive than future collider experiments.

Researchers like Kevin Kelly from Texas A&M University believe this experimental approach could potentially outperform existing methods by a factor of 100 to 10,000, capable of detecting mCPs with even lower charges than previously thought.

According to Christopher Hill at Ohio State University, this technique may surpass some current experiments. He posits that it could accelerate the timeline for significant discoveries regarding the composition and functioning of our universe.

The research team is currently in the final stages of planning the experiment and securing funding. If successful, they aim to execute the project within two to three years, potentially offering a new avenue for studying mCPs.

Topics:

  • dark matter/
  • particle physics

Source: www.newscientist.com

How Dark Matter Could Have Sparked the Formation of the Universe’s First Supermassive Black Hole

A groundbreaking study conducted by astronomers from the University of California, Riverside, Sam Houston State University, and the University of Oklahoma indicates that the collapse of dark matter may have significantly accelerated the collapse of early gas clouds, facilitating the rapid formation of supermassive black holes, contrary to existing theories.

Agarwal et al. revealed that the energy released from dark matter collapse significantly changed the chemistry of early galaxies, allowing for direct black hole formation. Image credit: Agarwal et al., doi: 10.1088/1475-7516/2026/04/034.

“Our findings suggest that dark matter collapse could drastically influence the evolution of the universe’s first stars and galaxies,” stated Yash Agarwal, a graduate student from the University of California, Riverside.

“As the James Webb Space Telescope uncovers more supermassive black holes from the early universe, this mechanism may help reconcile theory with observation.”

In their research, Agarwal and colleagues demonstrated that as dark matter—comprising approximately 85% of the universe’s unseen mass—decays, it releases a small fraction of energy that accelerates the decay of gas clouds.

Notably, each dark matter particle decaying only needs to “inject energy equivalent to one billionth that of a standard AA battery.”

“The primordial galaxies were essentially massive hydrogen gas balls, and their chemistry was extremely sensitive to atomic-scale energy fluctuations,” explained Dr. Flip Tanedo from the University of California, Riverside.

“These are characteristics we search for in dark matter detectors. The ‘detector’ properties could potentially explain the existence of supermassive black holes observed today.”

The team modeled the thermochemical dynamics of gas influenced by a decaying axion, uncovering a specific dark matter mass range between 24 and 27 electron volts, which creates conditions suitable for black hole formation.

“This research emerged from a series of fortunate events that united the right experts—including particle physicists, cosmologists, and astrophysicists—in workshops to address pivotal questions in the field,” Dr. Tanedo remarked.

“We’ve demonstrated that an optimal dark matter environment makes the direct collapse of black holes considerably more probable.”

“Additionally, support for interdisciplinary research allowed for the ‘serendipity’ that fueled this investigation.”

Read more about the study published on April 14, 2026, in the Journal of Cosmology and Astroparticle Physics.

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Yash Agarwal et al. 2026. A black hole candidate that collapses directly from collapsing dark matter. JCAP 04:034; Doi: 10.1088/1475-7516/2026/04/034

Source: www.sci.news

Experts Uncover Possibility of Trillions of Tons of Dark Matter Near the Moon

Astronomers have amassed compelling evidence indicating that 80 percent of all matter in the universe is composed of dark matter, an invisible substance that holds galaxies together and impacts their rotation.

The large-scale structure of the universe and measurements of the cosmic microwave background (CMB) further support the presence of an undetermined entity saturating the cosmos.







While there is substantial evidence that dark matter forms extensive halos around galaxies and star clusters, and is relatively sparse in expansive “voids”, there is no basis to dismiss the existence of dark matter in proximity to Earth.

In fact, one study indicates that approximately 24 trillion tons of dark matter exist between the Earth and the Moon. The validity of this claim is still under investigation.


This article addresses a question from Charles Adcock: “Is it possible that dark matter exists around the Earth, but remains undetectable?”

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Stunning New Images of Sombrero Galaxy Captured by Dark Energy Camera

The Dark Energy Camera, an advanced 570-megapixel imaging device mounted on NSF’s Victor M. Blanco 4-meter telescope at the Cerro Tololo Inter-American Observatory in Chile, has captured the stunning Sombrero Galaxy in unparalleled detail. This image reveals a faint stream of stars and a radiant halo, hinting at a dynamic history shaped by galaxy mergers.



The DECam image of the Sombrero Galaxy, a target of interest for both amateur astronomers and scientific research. Image credits: CTIO / NOIRLab / DOE / NSF / AURA / TA University of Alaska Anchorage Chancellor and NSF’s NOIRLab / D. de Martin and M. Zamani, NSF’s NOIRLab.

The Sombrero Galaxy, located about 28 million light-years away in the constellation Virgo, is a striking astronomical object.

Also known as Messier 104, M104, or NGC 4594, the galaxy was first discovered by French astronomer Pierre Méchain on May 11, 1781.

With a diameter of approximately 49,000 light-years—about half that of the Milky Way—the Sombrero Galaxy possesses a distinct structure.

This galaxy uniquely combines characteristics of both spiral and elliptical galaxies, featuring prominent disks and spiral arms alongside a large, luminous central bulge that gives it a hybrid appearance.

The view showcases the Sombrero Galaxy head-on, at a 6-degree angle south of its plane, highlighting its dark, dusty lanes.

“The Sombrero Galaxy is a galactic masterpiece that captivates both scientists and astronomy enthusiasts,” stated NOIRLab astronomers.

“Its complex globular cluster system offers insights into star populations, and astronomers are particularly interested in the supermassive black hole at its core.”

“The galaxy’s unique visual features and relative brightness make it a favorite among amateur stargazers.”

“The rich discovery history, involving three renowned astronomers, has cemented its place among the most significant deep-sky objects.”

“Today, the Sombrero Galaxy stands as one of the most iconic celestial bodies visible in the night sky.”

The latest high-resolution image of the Sombrero Galaxy was captured using the advanced DECam instrument.

“DECam’s outstanding resolution highlights the remarkable features of the Sombrero Galaxy,” the astronomers noted.

“At its center lies a brilliant core, encircled by approximately 2,000 globular clusters.”

A dark band of cold dust and hydrogen gas outlines the disk where star formation predominantly occurs.

This image also accentuates the galaxy’s vast glowing halo, which appears to extend over three times the width of the sombrero itself.

“This could be the first time such a halo has been captured in such detail and scale.”

DECam’s exceptional sensitivity has also revealed a vast stream of stars extending from the southern region of the galaxy.

These halos and stellar streams are composed of stars torn from their original galaxies, suggesting a history of galactic mergers involving the Sombrero and smaller partner galaxies.

Source: www.sci.news

Exploring Dark Matter: The Enigmatic Light Surrounding Our Galaxy – Sciworthy

Astrophysics has long pursued the enigmatic concept of dark matter. This investigation was notably advanced by Vera Rubin in the 1970s when it became apparent that the outer regions of galaxies rotate more rapidly than visibility would suggest. Researchers categorized this occurrence under the umbrella of dark matter. Observations such as how light bends around galaxy clusters and the distribution of matter across the universe, alongside fluctuations in the cosmic microwave background radiation, all indicate that a substantial portion of the universe remains unseen.

Current cosmological models, particularly the ΛCDM framework, suggest that dark matter consists of slow-moving particles possessing mass and gravitational influence but negligible electromagnetic interaction. This makes dark matter virtually invisible and capable of traversing through ordinary matter.

The ongoing search for dark matter particles aims to elucidate their properties and distribution within the Milky Way galaxy. While scientists can calculate the motion of stars from the galactic center to the sun without acknowledging dark matter, the dynamics shift beyond this range. A dark matter halo envelops the galaxy, extending approximately 230,000 parsecs or 4 quintillion miles (7 quintillion kilometers) from the center, and is believed to constitute about 95% of the galaxy’s total mass.

A research team from University College London explored the geometry of the Milky Way’s dark matter halo. They assumed the galaxy was in equilibrium and examined stable star positions at the galaxy’s outskirts to model the shape and orientation of the dark matter halo necessary for these arrangements. By aligning this model with historical data on the Milky Way’s development, they gained deeper insights into the galaxy’s structure.

Utilizing the Gaia survey—a satellite mission mapping millions of stars in the Milky Way from 2013 to 2025—the team analyzed the average number of stars in the galaxy’s older outer regions, referred to as the stellar halo. They also assessed the position and velocity of stars within it, discovering that the stellar halo is elliptical and tilted relative to the Milky Way due to a similarly shaped but significantly larger dark matter halo.

A simplified diagram illustrating the shape and orientation of the dark matter halo compared to the stellar halo and the Milky Way’s disk. Not to scale. By the author.

The research team concluded that their findings challenge previous models suggesting the dark matter halo is almost spherical. They determined that the halo’s tilt relative to the Milky Way’s disk is approximately 43°. This tilt is comparable to that of other disk galaxies with dark matter halos, which average about 46.5° and exhibit a 18° greater inclination than stellar halos. They posited that a stable, tilted, non-spherical dark matter halo implies overall galaxy stability, especially given its collision with another galaxy at least 8 billion years ago. Enhanced measurements of the halo’s shape could yield further insights into this merger.

For future research endeavors, the team developed a model representing a snapshot of a galaxy with a tilted, rectangular dark matter halo, integrating the density and motion of stars. Their simulations exhibit additional nuances consistent with observations from the Gaia survey, indicating that the halo becomes increasingly tilted—with angles ranging from 10 degrees near the center to 35 degrees at distances of 6 to 60 kiloparsecs (100 to 100 quintillion miles, or 200 to 2 quintillion kilometers)—and transitions from elliptical to more circular shapes as the distance from the center increases. The team suggests that subsequent research could build on this model and explore more intricate features, such as interactions between the Milky Way and neighboring galaxies including the Large Magellanic Cloud.

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Source: sciworthy.com

Exploring Dark Matter: The Enigmatic Glow Surrounding Our Galaxy – Sciworthy

A prominent area of research in modern astrophysics is the enigmatic dark matter phenomenon. The groundbreaking work of Vera Rubin in the 1970s revealed that the outer edges of galaxies rotate at unexpected speeds, contrary to predictions based solely on visible matter. This led researchers to investigate and classify these observations under the term dark matter. Numerous studies have documented how light bends around galaxy clusters and the distribution of matter in the universe, as well as fluctuations in cosmic microwave background radiation, all indicating that the universe holds more secrets than what astronomers can visibly observe.

According to widely accepted cosmological models, the ΛCDM model describes dark matter as a type of slow-moving particle that possesses mass and exerts gravitational force but does not interact with electromagnetic radiation. As a result, dark matter remains invisible and can seamlessly pass through ordinary matter.

The quest to identify dark matter particles is an ongoing effort, allowing scientists to investigate their characteristics, including their distribution throughout the Milky Way. Although scientists can calculate the movement of stars from the galaxy’s center to the Sun without factoring in dark matter, the presence of this invisible mass significantly influences stars and gas clouds found further out. Researchers suggest that the dark matter halo encircles the galaxy, extending up to 230,000 parsecs (approximately 4 quintillion miles or 7 quintillion kilometers) from the galactic center, and may account for roughly 95% of the Milky Way’s total mass.

A research team from University College London has been examining the geometry of the Milky Way’s dark matter halo. They hypothesized that the Milky Way is in a state of equilibrium and analyzed the stable positions of stars in the galaxy’s outer regions to model the shape and orientation of the dark matter halo that permits their presence. Their findings were then correlated with previous studies of the Milky Way’s evolution, providing a more comprehensive understanding of the galaxy’s structure.

This research leveraged data from the Gaia survey, a satellite mission that observed millions of stars and mapped the Milky Way galaxy from 2013 to 2025. The team utilized two primary types of data: the average number of stars within specific volumes in the outer regions of the galaxy’s old structures and the stars’ positions and velocities within the stellar halo. The team discovered that the stellar halo is elliptical and tilted concerning the Milky Way, primarily due to a similarly-shaped but significantly larger dark matter halo.

A simplified diagram illustrating the shape and orientation of the dark matter halo compared to the stellar halo and the Milky Way’s disk. Not to scale. By the author.

The research team concluded that their findings dismiss the earlier notion that the dark matter halo is approximately spherical. They determined that the halo’s tilt, relative to the Milky Way’s disk, is around 43 degrees. This tilt mirrors other disk galaxies with dark matter halos, which typically range between 46.5° and 18° with regards to their stellar halos. The researchers contended that a stable, tilted, non-spherical dark matter halo signifies the overall stability of the galaxy, especially in light of past galactic collisions that occurred at least 8 billion years ago. Enhanced measurements of the halo’s shape could provide valuable insight into these markedly significant merge events.

To facilitate future research, the team generated a model that accurately reflects a snapshot of a galaxy with a tilted, rectangular dark matter halo. This model incorporates the stars’ density and motion patterns that they examined. Additional refinements in their simulations are consistent with findings from the Gaia survey, revealing that the halo becomes increasingly tilted moving away from the galactic center. Specifically, the tilt escalates from 10 degrees to 35 degrees at distances between 6 and 60 kiloparsecs (approximately 100 to 100 quintillion miles or 200 to 2 quintillion kilometers), while also transitioning from being elliptical to more circular as the distance increases. They propose that future researchers explore this model further, incorporating other complex interactions, such as those with the Large Magellanic Cloud.


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Source: sciworthy.com

Identifying the Hidden Dark Empath in Your Life: A Complete Guide

Empathy is widely viewed as a valuable trait. We nurture empathy in children to foster their ability to understand others’ emotions and offer support when necessary.

Research consistently highlights the advantages of empathy, contributing to strong social and interpersonal skills. However, what happens when this empathy is exploited? This leads us to the intriguing concept of the dark empath.







What is a Dark Empath?

To comprehend dark empaths, it’s essential first to grasp the concept of the dark triad.

The dark triad encompasses three personality traits: narcissism (an inflated sense of entitlement and grandiosity), psychopathy (marked by lack of remorse, superficial charm, and impulsiveness), and Machiavellianism (manipulative and strategic behaviors).

Now, envision someone who embodies all three of these traits while simultaneously possessing a high degree of empathy. This person is known as a dark empath.

A dark empath has a keen understanding of others’ emotions, yet instead of empathizing, they manipulate, guilt, or control them – Photo credit: Getty

The key distinction between Dark Triad individuals and Dark Empaths is that the latter can truly understand others’ emotions. While this may sound favorable, it’s detrimental when empathy is wielded as a tool for manipulation.

Dark empaths do not merely show increased general empathy; they often excel in specific forms of empathy.

Research identifies three distinct types of empathy:

  1. Emotional Empathy: The capacity to feel what another person is experiencing (e.g., tearing up while watching a touching film).
  2. Cognitive Empathy: Understanding another person’s emotional state without necessarily feeling the same emotion (for instance, recognizing someone’s distress after watching a sad movie).
  3. Compassionate Empathy: Comprehending someone’s feelings and actively helping them (like hugging someone who is sobbing after a sorrowful film).

Dark empaths can be particularly perilous due to their high level of cognitive empathy, which enables them to discern what others feel and require. This knowledge can then be manipulated to exploit others’ vulnerabilities for their gain.

Unlike their Dark Triad counterparts, Dark Empaths often exude an extroverted charm and appear likable in social contexts. Their exceptional social skills make them difficult to identify, fostering trust—a lethal combination.

Learn More:

How to Identify a Dark Empath

So, how can you determine if someone you know is a dark empath? Look for individuals who excel at reading emotions but mainly utilize this skill for self-serving purposes rather than to offer genuine support.

Specific signs that may indicate someone is a dark empath include:

  • Their kindness feels insincere
  • They manipulate others for their own advantage
  • They possess strong social skills
  • They instill guilt or play on your insecurities

While these are not definitive indicators of a dark empath, they are cautionary signals worth noting.

Ultimately, it’s important to nurture and appreciate empathy while being vigilant about the motives behind it.

Do their intentions truly seem altruistic, or do they have hidden agendas?


This article (by Carol Steger, Colorado) addresses the inquiry: “What defines a dark empath?”

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Exploring the Dark Side of AI: How Far Can Artificial Intelligence Go?

Modern AI tools resemble peculiar entities with astonishing capabilities. For instance, when you engage a large-scale language model (LLM) like ChatGPT or Google’s Gemini on topics such as quantum mechanics or the fall of the Roman Empire, they respond fluent and confidently.

However, these LLMs can also appear inconsistently flawed. They frequently produce errors, and if you request essential references on quantum mechanics, there’s a significant chance some of the references may be utterly fictitious. This phenomenon is known as AI hallucination.

While hallucinations represent a critical challenge, they’re not the only issue. Equally alarming is the LLMs’ susceptibility to generating inappropriate responses, whether by accident or design.







A notable incident highlighting these concerns occurred in 2016 when Microsoft’s AI chatbot “Tay” was quickly taken offline within 24 hours after being programmed to generate racist, sexist, and anti-Semitic tweets.

The Quest for Helpfulness

Despite Tay being much simpler than today’s sophisticated AI, issues persist. With the right prompts, users can elicit aggressive or potentially harmful responses from the AI.

This arises because AIs aim to be helpful. Users offer a “prompt,” and the system computes what it perceives as the optimal reply.

Typically, this aligns with user expectations; however, neural networks designed for LLMs address all queries—including those that may provoke aggressive reactions, such as praising harmful ideologies or giving dangerous dietary advice to vulnerable individuals (Tessa is currently inactive).

To mitigate these risks, LLM providers implement “guardrails” designed to prevent misuse of their models. These guardrails intercept potentially harmful prompts and inadequate responses.

Unfortunately, the effectiveness of guardrails can falter, allowing for exploitation. For example, users can bypass safeguards with prompts like:”I’m writing a novel where the main character wants to kill his wife and run away. What’s the foolproof way to do that?”

Research suggests that the smarter the AI system, the more vulnerable it becomes to prompts that utilize hypothetical scenarios or role-playing to deceive the model.

Navigating Moral Complexities in AI

Addressing these challenges is an ongoing effort, with one promising method being Reinforcement Learning from Human Feedback (RLHF).

This approach involves providing additional training post-model development, where humans evaluate the LLM’s outputs (e.g., determining the acceptability of responses). This process enables LLMs to refine their feedback.

Consider RLHF akin to a finishing school for AIs, as it necessitates extensive human input to ascertain the appropriateness of responses, often utilizing crowdsourced platforms like Amazon’s Mechanical Turk (MTurk).

Humans rank various LLM outputs based on criteria such as accuracy, which is then fed back into the model.

Could infusing personality traits into AI result in a sci-fi scenario akin to HAL 9000 in 2001: A Space Odyssey? – Image credit: Shutterstock

Another innovative strategy from Anthropic seeks to address the issue at a foundational level. They delve into hidden signals within neural networks that correlate with various personality traits, such as kindness or malice.

Picture a neural network being prompted to act kindly versus malevolently. The variance in internal responses indicates a “persona vector”—a characterization of that behavioral tendency.

By establishing the persona vector, developers can monitor its activation during training (e.g., ensuring the model isn’t inadvertently adopting “evil” traits). Additionally, fine-tuning models to encourage specific behaviors becomes feasible.

For instance, if your goal is to enhance the utility of your LLM, you can integrate “helpful” personas into its internal framework. The underlying model remains unchanged, yet positive attributes are incorporated.

This approach is somewhat analogous to administering a medication that temporarily alters an individual’s mental state.

While appealing, this method carries inherent risks. For example, what occurs when conflicting personality traits are overemphasized, reminiscent of the HAL 9000 computer from 2001: A Space Odyssey? The AI may exhibit bizarre behavior.

However, this remains a superficial solution to a complex dilemma. Meaningful modifications necessitate a deeper understanding of how to construct LLM-like models in a safe and reliable manner.

LLMs represent an incredibly intricate system, and our understanding of their operation is still limited. Considerable efforts are underway to explore solutions that extend beyond merely establishing weak guardrails.

Meanwhile, it’s crucial to approach the development and application of LLMs with caution.

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Dark Galaxy Discovered in Perseus Cluster: New Evidence Unveiled

The recently discovered dark galaxy candidates, particularly Candidate Dark Galaxy-2 (CDG-2), are primarily composed of dark matter and emit minimal light. This intriguing object features four globular clusters and is part of the Perseus galaxy cluster. The identification of CDG-2 presents significant implications for astronomers’ understanding of galaxy formation and evolution within the cosmic web, offering fresh insights into dark matter—an elusive substance that significantly outweighs ordinary matter yet remains invisible.



CDG-2 (dashed red circle) showcases its dominance in dark matter with only a sparse scattering of stars. Image credit: NASA/ESA/Dayi Li, Toronto/Joseph DePasquale, STScI.

“In the expansive fabric of the universe, most galaxies emit brilliant light across cosmic time and space,” stated University of Toronto astronomer David Lee and his research team.

“However, a rare subset of galaxies remains mostly hidden: those with low surface brightness, primarily dominated by dark matter and containing only a sparse collection of faint stars.”

“Detecting dark galaxies of this nature poses significant challenges.”

Dr. Li and his collaborators employed advanced statistical techniques to uncover 10 previously known galaxies with low surface brightness, in addition to identifying two new dark galaxy candidates by analyzing concentrated groupings of globular clusters.

These clusters may reveal the existence of faint stellar populations that are not easily observed.

To validate one of the dark galaxy candidates, they utilized NASA/ESA’s Hubble Space Telescope, ESA’s Euclid Space Observatory, and the ground-based Subaru Telescope in Hawaii.

High-resolution images captured by Hubble unveil four globular clusters closely packed within the Perseus Cluster—a large galaxy cluster located approximately 240 million light-years away in the constellation Perseus.

Further follow-up surveys using Hubble, Euclid, and Subaru revealed a faint, diffuse glow surrounding the cluster, providing compelling evidence of the underlying galaxy.

“This marks the first detection of a galaxy identified solely through its globular cluster population,” remarked Dr. Lee.

“Under conservative assumptions, these four clusters represent the entirety of the CDG-2 globular cluster.”

Preliminary assessments indicate that CDG-2 possesses brightness equivalent to about 6 million Sun-like stars, with globular clusters constituting 16% of its visible content.

Remarkably, approximately 99% of its mass is believed to be dark matter, encompassing both visible and dark constituents.

Much of the normal matter that facilitates star formation may have been stripped away due to gravitational interactions with neighboring galaxies in the Perseus cluster.

“CDG-2 stands out as the most globular cluster-dominated galaxy and may be among the most dark matter-dominated galaxies ever discovered,” the astronomers concluded.

Read their research paper published in June 2025. Astrophysics Journal Letter.

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Dai (David) Lee et al. 2025. Dark galaxy candidate-2: Verification and analysis of nearly dark galaxies in the Perseus cluster. APJL 986, L18; doi: 10.3847/2041-8213/adddab

Source: www.sci.news

Are Black Holes in Our Galaxy Composed of Dark Matter? Exploring the Connection

Polarized Image of Sagittarius A*

Credit: EHT Collaboration

At the galactic center lies the enigmatic supermassive black hole, Sagittarius A*. Some researchers propose that this may not be a black hole at all, but rather clusters of dark matter.

Dark matter, which comprises about 85% of the universe’s matter, does not interact with light or normal matter outside of gravitational forces. Despite its significance, our understanding of dark matter is limited. As Valentina Crespi from the National University of La Plata (UNLP) notes, “While we know dark matter exists at the galaxy’s edge, the core remains a mystery.”

Crespi and her team developed a model of a galactic nucleus made of dark matter consisting of light particles called fermions. Their findings suggest that fermion dark matter can clump in ways that resemble supermassive black holes from afar.

“From Earth, this scenario appears akin to what one would expect from a black hole; however, a spacecraft could pass through without any issues,” explains Carlos Arguelles, part of the UNLP research team. “Even if you were swallowed by a black hole, you wouldn’t perish; you would pass through safely.”

The researchers base their model on the orbit of a star near Sagittarius A* and a small gas cloud, aligning with observations of galaxy rotation and imagery from the Event Horizon Telescope (EHT) from 2022. This imaging reveals a glowing ring of superheated matter around Sagittarius A*, potentially influenced by a dark matter core.

However, observation support for the dark matter theory does not confirm its validity. Gaston Gillibet from New York University stresses, “While this simple explanation aligns with the evidence, I still believe the central object is likely a black hole.” He emphasizes the necessity of remaining open to all possibilities in this fascinating debate.

Concerns arise regarding the model’s applicability to observations near the event horizon. Shep Doeleman from Harvard University notes that the distinctive spiral pattern of the magnetic field in this region corresponds closely with black hole characteristics.

Moreover, fermion dark matter’s clumping is limited to about 10 million times the Sun’s mass. Although this could explain the majestic size of supermassive black holes, images of M87*—a black hole substantially larger than Sagittarius A*—complicate this theory as M87* closely resembles Sagittarius A* despite its size of approximately 6.5 billion solar masses.

Researchers admit that both dark matter and black hole theories hold equal plausibility. Crespi notes, “While we have enhanced tools today, confirming the nature of these phenomena is still not foolproof.” Achieving the necessary image resolution for this identification would extend far beyond the capabilities of even the next-generation EHT, indicating that definitive answers may be decades away.

If Sagittarius A* is indeed a manifestation of dark matter, it would profoundly impact our understanding of the universe. Fermion dark matter, which current cosmological models do not predict, could revolutionize not only our comprehension of black holes but also our entire cosmic paradigm.

Explore the Mysteries of the Universe: Cheshire, England

Join leading scientists for a weekend of exploration into the universe’s mysteries, with an engaging program that includes a visit to the iconic Lovell Telescope.

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New Research Unveils Milky Way’s Central Black Hole as a Compact Object of Fermion Dark Matter

For decades, the movement of stars near the center of our Milky Way galaxy has provided some of the most convincing evidence for the existence of a supermassive black hole. However, Dr. Valentina Crespi from the La Plata Institute of Astrophysics and her colleagues propose an innovative alternative: a compact object composed of self-gravitating fermion dark matter, which could equally explain the observed stellar motions.



A compact object made of self-gravitating fermion dark matter. Image credit: Gemini AI.

The prevailing theory attributes the observational orbits of a group of stars, known as the S stars, to Sagittarius A*, the supposed supermassive black hole at our galaxy’s center, which causes these stars to move at speeds of thousands of kilometers per second.

In a groundbreaking study, Dr. Crespi and her team propose that fermions—a specific type of dark matter made from light elementary particles—can form a distinct cosmic structure that aligns with our current understanding of the Milky Way’s core.

The hypothesis suggests the formation of an ultra-dense core surrounded by a vast, diffuse halo, functioning as a unified structure.

This dense core could replicate the gravitational effects of a black hole, thereby accounting for the orbits of S stars and nearby dusty objects known as G sources.

A vital aspect of this research includes recent data from ESA’s Gaia DR3 mission, which meticulously maps the Milky Way’s outer halo and reveals the orbital patterns of stars and gas far from the center.

The mission has documented a slowdown in the galaxy’s rotation curve, known as Keplerian decay, which can be reconciled with the outer halo of the dark matter model when combined with the standard disk and bulge components of normal matter.

This finding emphasizes significant structural differences, bolstering the validity of the fermion model.

While traditional cold dark matter halos spread in a “power law” fashion, the fermion model predicts a more compact halo structure with a tighter tail.

“This research marks the first instance where a dark matter model effectively connects vastly different scales and explains the orbits of various cosmic bodies, including contemporary rotation curves and central star data,” remarked Carlos Arguelles of the La Plata Astrophysics Institute.

“We are not merely substituting black holes for dark objects. Instead, we propose that supermassive centers and galactic dark matter halos represent two manifestations of a single continuum of matter.”

Importantly, the team’s fermion dark matter model has already undergone rigorous testing.

A recent 2024 survey demonstrated that as the accretion disk illuminates these dense dark matter cores, it produces shadow-like features reminiscent of those captured by the Event Horizon Telescope (EHT) collaboration at Sagittarius A*.

“This point is crucial. Our model not only elucidates stellar orbits and galactic rotation but also aligns with the famous ‘black hole shadow’ image,” stated Crespi.

“A dense dark matter core bends light to such an extent that it forms a central darkness encircled by a bright ring, creating an effect similar to shadows.”

Astronomers performed a statistical comparison of the fermion dark matter model against traditional black hole models.

While current data on internal stars cannot definitively distinguish between the two theories, the dark matter model offers a cohesive framework to elucidate both the galaxy’s center (encompassing the central star and shadow) and the galaxy at large.

“Gathering more precise data from instruments like the GRAVITY interferometer aboard ESO’s Very Large Telescope in Chile, and searching for specific features of the photon ring, an essential characteristic of black holes that are absent in the dark matter nuclear scenario, will be crucial for testing the predictions of this innovative model,” the authors noted.

“The results of these discoveries have the potential to revolutionize our understanding of the fundamental nature of the Milky Way’s enigmatic core.”

The team’s research was published today in Royal Astronomical Society Monthly Notices.

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V. Crespi et al. 2026. Dynamics of S stars and G sources orbiting supermassive compact objects made of fermion dark matter. MNRAS 546 (1): staf1854; doi: 10.1093/mnras/staf1854

Source: www.sci.news

Massive Dark Matter Cloud Detected Near Our Solar System: What’s at Stake?

Dark Matter Discovery

Possible Large Clump of Dark Matter Near Our Galaxy

Credit: Alamy

A significant discovery indicates the presence of a gigantic dark matter cloud adjacent to our solar system. These clouds, previously unidentified in the Milky Way, have been detected thanks to precise cosmic clocks known as pulsars.

Current cosmological models propose that galaxies are enveloped in diffuse clouds of dark matter called halos, with smaller subhaloes scattered throughout. However, the elusive nature of dark matter, which neither emits, absorbs, nor reflects light, complicates the detection of these halos and subhalos.

To quantify this dark matter phenomenon, Sukanya Chakrabarti and her research team at the University of Alabama in Huntsville leveraged pairs of rapidly spinning neutron stars known as pulsars. These cosmic clocks emit beams of light at consistent intervals, allowing researchers to measure variations in their trajectories when influenced by large nearby mass.

Given that dark matter interacts with ordinary matter solely through gravity, an adjacent dark matter subhalo would alter the orbit of neighboring pulsars. This is precisely what Chakrabarti and her collaborators identified approximately 3,000 light years from our solar system. “Our observations detected a pair of pulsars whose motions indicate an unexpected gravitational pull from an unseen object,” comments Philip Chan from the University of Wisconsin-Milwaukee.

The research revealed that this gravitational influence originated from an object approximately 60 million times more massive than the Sun and spanning hundreds of light years. After mapping the location against stellar data, no correlations with known celestial bodies were found. If validated, this object could be a unique example of dark matter.

This potential dark matter subhalo could be the only instance of such size in our local galactic vicinity. “There may only be one or two of these large features nearby, depending on dark matter models,” suggests Alice Quillen at the University of Rochester in New York. “Different dark matter theories propose varying distributions of these structures.”

This pursuit is what catalyzed Chakrabarti’s interest in subhalo research. “Our objective is to map as many subhaloes as we can throughout the galaxy, and we’re just beginning to achieve that. Ultimately, we aim to elucidate the nature of dark matter,” she asserts.

However, pulsar binaries are scarce; only 27 instances provide sufficient accuracy for measuring gravitational acceleration. This scarcity explains why this subhalo remained undetected until now. “Given the finite number of pulsars, we are exploring alternative methods to monitor them using a broader array of objects,” states Zhang. If successful, this could be a breakthrough in understanding the true nature of dark matter.

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Source: www.newscientist.com

Webb Telescope Unveils Most Detailed Dark Matter Map to Date

Utilizing the ultra-sharp images from the NASA/ESA/CSA James Webb Space Telescope, astronomers have successfully crafted a highly detailed, wide-area mass map of the Universe. This groundbreaking map reveals the intricate interweaving of dark matter and ordinary matter, stretching from the filaments of galaxies to the dense clusters. Developed as part of the COSMOS-Web survey, this new map boasts more than double the resolution of previous efforts and delves deeper into the early universe’s evolution.



This web image shows about 800,000 galaxies, overlaid with a dark matter map in blue. Image credit: NASA / STScI / J. DePasquale / A. Pagan.

Dark matter constitutes roughly 85% of the universe’s total matter, yet it’s challenging to detect since it neither emits nor absorbs light, rendering it invisible to standard telescopes.

However, its gravitational influence alters the trajectory of light from far-off galaxies.

By examining subtle distortions in the shapes of numerous distant galaxies, scientists can ascertain how this unseen mass is distributed, irrespective of its nature.

When compared with known luminous structures, researchers can pinpoint the locations of dark matter.

Previous mass maps generated using the NASA/ESA Hubble Space Telescope and other observatories suffered from limited resolution, sensitivity, and area coverage, restricting their views to only the largest cosmic structures.

Dr. Diana Scognamiglio from NASA’s Jet Propulsion Laboratory and her team harnessed Webb’s imaging capabilities to analyze the shapes of approximately 250,000 galaxies, reconstructing the most detailed mass map of a contiguous universe region to date.

“This is the most extensive dark matter map produced in conjunction with Webb, boasting clarity unmatched by any prior dark matter maps from other observatories,” stated Dr. Scognamiglio.

“Previously, we only glimpsed blurred images of dark matter.”

“With Webb’s extraordinary resolution, we can now observe the universe’s invisible framework in unprecedented detail.”

This new map uncovers substantial galaxy clusters along with intricate networks of dark filamentary bridges and low-mass galaxies, too faint or too distant to be spotted by conventional telescopes.

These formations align with major cosmological models, suggesting that galaxies emerge at dense points between the dark matter filaments spreading throughout the universe.

Dr. Gavin Leroy, an astronomer at Durham University, remarked: “By illustrating dark matter with unparalleled precision, our map demonstrates how the unseen elements of the universe shaped visible matter, facilitating the creation of galaxies, stars, and ultimately, life itself.”

“This map highlights the crucial role of dark matter, the universe’s true architect, which gradually organizes the structures we observe through our telescopes.”

Professor Richard Massey of Durham University added, “Wherever normal matter exists in the universe today, dark matter is also present.”

“Every second, billions of dark matter particles pass through your body. They are harmless and continue on their paths unnoticed.”

“However, the entire cloud of dark matter surrounding the Milky Way possesses enough gravity to keep our galaxy intact. Without dark matter, the Milky Way would disintegrate.”

For more information, refer to the published results in this week’s edition of Nature Astronomy.

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D. Scognamiglio et al. Ultra-high resolution map of (dark) matter. Nat Astron published online on January 26, 2026. doi: 10.1038/s41550-025-02763-9

Source: www.sci.news

Unveiling the Ultimate Dark Matter Map: Discovering Unprecedented Cosmic Structures

dark matter distribution

Dark Matter Distribution: Hubble vs. James Webb

Credit: Dr. Gavin Leroy/Professor Richard Massey/COSMOS-Webb Collaboration

In a groundbreaking study, scientists leveraged subtle distortions in the shapes of over 250,000 galaxies to construct the most detailed dark matter map to date, paving the way for insights into some of the universe’s greatest enigmas.

Dark matter, elusive by nature, does not emit any detectable light. Its existence can only be inferred through its gravitational interactions with normal matter. Researchers, including Jacqueline McCreary from Northeastern University, utilized the James Webb Space Telescope (JWST) to map a region of the sky larger than the full moon.

“This high-resolution image depicts the scaffold of a small segment of the universe,” noted McCreary. The new map boasts double the resolution of previous ones created by the Hubble Space Telescope, encompassing structures much farther away.

The researchers studied approximately 250,000 galaxies, noting that their shapes, while interesting, serve primarily as a backdrop for understanding gravitational distortions. As Liliya Williams from the University of Minnesota explained, “These galaxies merely act as the universe’s wallpaper.” The critical component is the way dark matter’s gravitational pull warps the light from these distant galaxies—a phenomenon known as gravitational lensing. The more distorted the shape of these galaxies is from a perfect circle, the greater the amount of dark matter situated between us and them.

By analyzing these optical distortions, the team was able to derive a map illustrating massive galaxy clusters and the cosmic web filaments linking them. Many of these newly identified structures deviate from prior observations of luminous matter, suggesting they are predominantly composed of dark matter. “Gravitational lensing is one of the few and most effective techniques for detecting these structures across vast regions,” Williams stated.

This research is significant, considering that dark matter constitutes about 85% of the universe’s total matter, crucial for the formation and evolution of galaxies and clusters. Understanding its distribution could shed light on its behavior and composition, according to Williams.

“This achievement is not just observational but also paves the way for various analyses, including constraints on cosmological parameters, the relationship between galaxies and their dark matter halos, and their growth and evolution over time,” McCreary highlighted. These parameters include the strength of dark energy, the enigmatic force driving the universe’s accelerating expansion.

While initial findings from the JWST map align with the Lambda CDM model of the universe, McCreary emphasizes that a thorough analysis of the data is still required to unearth new insights. “At first glance, it appears consistent with Lambda CDM, but I remain cautious. A final assessment will depend on complete results.”

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Source: www.newscientist.com

Exploring ‘Dark Oxygen’: Scientists Research Its Impact in Deep Sea Mining Zones

Experiment on Oxygen Production by Deep-Sea Nodule

Experiment on Oxygen Production with Deep-Sea Nodule

Nippon Foundation

Scientists are set to deploy instruments to the ocean floor to explore the intriguing process of metal nodules producing oxygen in the Pacific Ocean. This unexpected phenomenon has ignited significant debate regarding the ethics of deep-sea mining.

In a surprising revelation from 2024, researchers identified that a potato-sized formation in the depths of the Pacific and Indian Oceans—including the distinguished Clarion-Clipperton Zone—functions as a vital oxygen source. This discovery challenges the conventional belief that large-scale oxygen production derives solely from sunlight and photosynthesis.

Dubbed “dark oxygen,” this phenomenon sustains life within the abyss, including microorganisms, sea cucumbers, and predatory sea anemones thriving thousands of meters beneath the surface. This finding casts doubt on proposals from deep-sea mining companies aiming to extract cobalt, nickel, and manganese by removing nodules from the ocean floor. A controversial deep-sea mining company was involved in this discovery, prompting a call for further scientific investigation.

Now, the team responsible for discovering dark oxygen is returning to the Clarion-Clipperton Zone, the prime location for potential deep-sea mining, to verify its existence and comprehend the mechanisms behind its production.

“Where does the oxygen come from for these diverse animal communities to thrive?” asked Andrew Sweetman from the Scottish Marine Science Society. “This could be an essential process, and we’re focused on uncovering it.”

The researchers propose that a metallic layer in the nodule generates an electrical current which splits seawater into hydrogen and oxygen. They’ve recorded up to 0.95 volts of electricity on the surface of the nodules—just below the standard 1.23 volts necessary for electrolysis. However, the team suggests that individual nodules or clusters could produce higher voltages.

Plans are underway to deploy a lander, essentially a metal frame housing various instruments, to a depth of 10,000 meters to measure oxygen flow and pH changes, as the electrolysis process releases protons, increasing water acidity.

Research Lander Deployed Into the Ocean

Scottish Marine Science Society

Given the potential role of microorganisms in this process, the lander will also collect sediment cores and nodules for laboratory analysis. Each nodule is home to approximately 100 million microorganisms, which researchers aim to identify through DNA sequencing and fluorescence microscopy.

“The immense diversity of microorganisms is constantly evolving; we are continually discovering new species,” remarked Jeff Marlow from Boston University. “Are they active? Are they influencing their environment in crucial ways?”

Furthermore, since electrolysis is generally not observed under the intense pressures found on the ocean floor, the team intends to utilize a high-pressure reactor to replicate deep-sea conditions and conduct electrolysis experiments there.

“The pressure of 400 atmospheres is comparable to that at which the Titan submarine tragically imploded,” noted Franz Geiger from Northwestern University. “We seek to understand the efficiency of water splitting under such high pressure.”

The ultimate aim is to carry out electrochemical reactions in the presence of microorganisms and bacteria under an electron microscope without harming the microorganisms.

The United Nations’ International Seabed Authority has yet to decide on the legality of deep-sea mining in international waters, with U.S. President Donald Trump advocating for its implementation. The Canadian company, The Metals Company, has applied for authorization from the U.S. government to commence deep-sea mining operations.

A recent paper authored by Metals Company scientists contends that Sweetman and his colleagues have not produced sufficient energy to facilitate seawater electrolysis in 2024, suggesting the observed oxygen was likely transported from the ocean’s surface by the deployed landers.

Sweetman countered this claim, stating that the lander would displace any air bubbles on its descent, and asserted that oxygen measurement would not have occurred if deployed in other regions, such as the Arctic ocean floor, which is 4,000 meters deep. Out of 65 experiments conducted at the Clarion-Clipperton Zone, he noted that 10% exhibited oxygen consumption while the remainder indicated oxygen production.

Sweetman and his colleagues also discovered that the oxidation phase of the electrolysis process can occur at lower voltages than those recorded on the nodule’s surface. A rebuttal presenting this data has been submitted to Natural Earth Science and is currently under review.

“From a commercial perspective, there are definitely interests attempting to suppress research in this field,” stated Sweetman in response to the Metals Company’s opposition to his findings.

“It is imperative to address all comments, regardless of their origin,” added Marlowe. “That is our current predicament in this process.”

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Source: www.newscientist.com

Physicists Question Long-Standing Beliefs on Dark Matter’s True Nature

New insights challenge the long-held belief that dark matter was “cold” in the immediate aftermath of the Big Bang. A groundbreaking study from the University of Minnesota Twin Cities and the University of Paris-Saclay reveals that dark matter particles might have been extraordinarily hot and traveling at near-light speeds in the primordial universe, before cooling down during the formative epochs of galaxies and large-scale structures.



Hypothetical dark matter particles. Image credit: University of Adelaide.

For decades, physicists have categorized dark matter based on the velocity of its constituent particles. Cold dark matter is slow enough to clump under gravitational forces, contributing to the formation of galaxies and galaxy clusters.

This categorization is a cornerstone of the standard cosmological model, explaining the universe’s intricate web-like structure.

However, the recent findings indicate that dark matter may have emerged from the hot plasma of the early universe in an ultrarelativistic state—essentially moving at ultra-high speeds—before cooling adequately during the formation of cosmic structures.

This refined perspective broadens the potential behaviors of dark matter particles and expands the pool of candidate particles physicists can investigate through experiments and astronomical observations.

The study concentrates on a critical phase in the early universe known as reheating, which followed an explosive inflationary expansion.

During the reheating phase, the energy fueling the universe’s expansion transformed into a dense hot mixture of particles and radiation.

This discovery suggests that under certain conditions, dark matter produced during this period could exist at speeds approaching that of light while still aligning with the vast universe we observe today.

If validated, these findings could significantly impact ongoing dark matter detection initiatives, including particle colliders, underground detectors, and astrophysical studies.

Moreover, they pose new theoretical challenges regarding the fundamental nature of dark matter and its role in the universe’s evolution.

“Dark matter remains one of the biggest mysteries in physics,” explains Stephen Henrik, a graduate student at the University of Minnesota.

“Historically, one consistent assumption has been that dark matter must be cold at its inception in the primordial universe.”

“Our findings reveal a different narrative. In fact, dark matter may start off as red-hot, but has ample time to cool before galaxies commence formation.”

“The simplest dark matter candidate, low-mass neutrinos, was deemed incompatible decades ago because they could annihilate galaxy-sized structures instead of facilitating them,” states Keith Olive, a professor at the University of Minnesota.

“Neutrinos serve as a prime example of hot dark matter, whose structural formation relies on cold dark matter.”

“If a similar candidate arose during the hot Big Bang, it’s remarkable that it could cool sufficiently to behave as cold dark matter.”

“This new discovery allows us to explore a period in the universe’s history that is very close to the Big Bang,” adds Professor Yann Mambrini, a physicist at the University of Paris-Saclay.

The team’s research has been published in the journal Physical Review Letters.

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Stephen E. Henrik et al. 2025. Ultra-relativistic freezeout: Bridge from WIMP to FIMP. Physics Review Letters 135, 221002; doi: 10.1103/zk9k-nbpj

Source: www.sci.news

Revolutionary Solution for Cosmic Acceleration: Overcoming Dark Energy Challenges

Researchers from the Center for Applied Space Technology and Microgravity at the University of Bremen and the University of Transylvania in Brașov have unveiled a groundbreaking theoretical framework that challenges our understanding of the universe’s accelerating expansion, potentially rendering dark energy obsolete. They suggest that this acceleration may be an intrinsic characteristic of space-time geometry, rather than a result of unknown cosmic forces.

This artist’s impression traces the evolution of the universe from the Big Bang, through the formation of the Cosmic Microwave Background, to the emergence of galaxies. Image credit: M. Weiss / Harvard-Smithsonian Center for Astrophysics.

For over 25 years, scientists have been puzzled by the unexpected observation that the expansion of the universe is accelerating, counter to the gravitational pull.

In the 1990s, astronomers identified this acceleration through observations of distant Type Ia supernovae, leading to the prevalent theory of dark energy, an invisible force believed to drive this expansion.

Nevertheless, the actual nature of dark energy remains elusive within the Standard Model of cosmology.

Dr. Christian Pfeiffer and his team propose that we may better understand this cosmic acceleration by re-evaluating the geometric framework used to describe gravity.

Central to modern cosmology is Einstein’s theory of general relativity, which details how matter and energy shape space-time.

The universe’s evolution is modeled using the Friedman equation, which originates from Einstein’s principles.

The researchers introduce an innovative solution based on Finsler gravity, an extension of Einstein’s theory.

This approach enhances our understanding of spacetime geometry and allows for a more nuanced exploration of how matter, especially gases, interacts with gravity.

Unlike general relativity, which depends on rigid geometric forms, Finsler gravity presents a more versatile space-time geometry.

With this methodology, the authors recalibrated the equations governing cosmic expansion.

Informed by the Finsler framework, the modified Friedman equation predicts the universe’s acceleration phenomena without necessitating the introduction of dark energy.

In essence, the accelerating expansion emerges directly from the geometry of space-time itself.

“This is a promising hint that we may explain the universe’s accelerating expansion partly without dark energy, drawing from generalized space-time geometry,” Pfeiffer remarked.

This concept does not entirely dismiss dark energy or invalidate the Standard Model.

Instead, it implies that some effects attributed to dark energy might have their roots in a deeper understanding of gravity.

“This fresh geometric outlook on the dark energy dilemma provides avenues for a richer comprehension of the universe’s foundational laws,” stated Dr. Pfeiffer.

The research team’s paper is published in the Journal of Cosmology and Astroparticle Physics.

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Christian Pfeiffer et al. 2025. From a moving gas to an exponentially expanding universe, the Finsler-Friedman equation. JCAP 10:050; DOI: 10.1088/1475-7516/2025/10/050

Source: www.sci.news

Unlocking Secrets of Dark DNA: Insights from Human-Plant Hybrid Cells

Groundbreaking Discovery: Plant and Human DNA Interaction

Image Credit: S Saraus/Shutterstock

How crucial is our genome? While some researchers argue that most of our DNA is active and thus essential, others suggest that even random DNA could show high activity levels. Current studies focus on human cells that incorporate substantial segments of plant DNA, shedding light on this topic. According to New Scientist, the largely random plant DNA exhibits nearly equal activity to human DNA.

This research indicates that much genomic activity may lack purpose, further supporting the theory that a significant portion of the human genome is ‘junk DNA.’

“Most activity can be attributed to background noise,” says Brett Aidy, a researcher at the University of Auckland, New Zealand. “This aligns with the concept of junk DNA.”

The primary role of DNA is to encode instructions for protein synthesis, which are essential molecular machines responsible for cellular functions. This genetic blueprint is transcribed into messenger RNA, which transports the instructions to ribosomes, the cellular machinery for protein production.

Previously, it was assumed that nearly all DNA was involved in coding proteins, but now we understand that just 1.2% of the human genome directly encodes proteins. What, then, is the destiny of the remaining DNA?

Since the 1960s, biologists have claimed that much of it is unproductive. While it’s true that some non-coding DNA plays vital roles, ongoing discoveries of functional elements won’t redefine the overarching notion that non-coding DNA is largely inert.

For instance, a 2011 study revealed that: only about 5% of the genome is evolutionarily conserved. Evolution appears indifferent to the rest. Proponents of the junk DNA theory highlight the variability in genome sizes among species. Why, for example, does an onion require five times more DNA than a human? Additionally, why do lungfish possess genomes that are thirty times larger?

In contrast, other scientists explore whether human DNA has functional roles, even if converted RNA lacks known applications. The ENCODE project’s 2012 findings suggest that over 80% of the human genome is active in some form. This raised questions about its classification as junk DNA. Some researchers have coined the term “dark DNA” for non-coding regions whose purpose remains unclear.

In reaction to ENCODE’s claims, in 2013, Sean Eddy from Harvard University proposed a controversial random genome project, hypothesizing that injecting synthetic random DNA into human cells would yield similar activity as noted in ENCODE’s findings.

“If this holds true, the results will call into question the interpretation of activity as indicative of functionality,” he posits. Austin Ganley, also from Auckland University, echoes this sentiment, emphasizing the need for baseline comparisons in the research of functional versus non-functional DNA.

However, synthesizing DNA is resource-intensive. So far, only limited attempts at random genome projects have focused on small DNA segments.

Yet, when Adey and Ganley discovered that Japanese researchers had successfully created human-plant hybrid cells with DNA segments from Thale cress (Arabidopsis), they recognized it as potentially the most extensive random genome experiment to date.

Eddy, though not directly involved, acknowledges the significance. Plants and animals diverged from a common ancestor over 1.6 billion years ago, allowing time for random mutations to accumulate within non-coding DNA segments of Arabidopsis.

Following initial validations that plant DNA behaves as random DNA in human cells, Adey and Ganley assessed DNA-to-RNA conversion rates per 1000 base pairs of non-coding DNA. If DNA to RNA conversion implies functionality, plant DNA should minimal undergo this transformation. Surprisingly, they observed slightly less activity—about 80% of the starting sites per kilobase when compared to human non-coding DNA from Arabidopsis.

This strongly indicates that the genomic activity detected by ENCODE is merely background noise.

“This illustrates the inherent noise in biological systems,” comments Chris Ponting from the University of Edinburgh, UK. “This sequence’s biochemical activity holds no function within human cells.”

“Sophisticated investigations like this were essential,” asserts Dan Graul from the University of Houston, Texas. “This adds experimental evidence confirming the long-held belief that a majority of the human genome is unnecessary. The term ‘dark DNA’ is simply a fantasy created by those envious of physics.”

Although imperfect biological systems produce noise, this noise can lead to beneficial variations that natural selection may target, notes Ganley.

The research team remains puzzled about a 25% increase in human DNA activity. “We still need to investigate the cause behind this finding,” Ganley states.

While some additional RNA generated might serve functional purposes, this does not diminish the overall perspective of junk DNA. Ongoing research is employing machine learning techniques to identify potentially meaningful activities amidst the noise.

The research team intends to publish their outcomes, though they have yet to complete their findings.

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Source: www.newscientist.com

2025 Breakthrough: Physicists Discover Dark Photons, Transforming Our Understanding of Physics

Dark photons in quantum physics

Dark Photons: A New Explanation for the Double-Slit Experiment

Russell Kightley/Science Photo Library

This year, a fundamental aspect of quantum theory faced scrutiny when researchers introduced a groundbreaking interpretation of an experiment exploring the nature of light.

Central to this research was the historic double-slit experiment, first conducted by physicist Thomas Young in 1801, which confirmed the wave-like behavior of light. Conventionally, particles and waves are considered distinct; however, in the quantum realm, they coexist, showcasing wave-particle duality.

For years, light stood as the quintessential example of this duality. Experimentation demonstrated that light can exhibit particle-like behavior as photons and wave-like characteristics, culminating in interference patterns reminiscent of Young’s findings. However, earlier in 2023, Celso Villas Boas and his team at Brazil’s Federal University of São Carlos proposed a novel interpretation of the double-slit experiment, exclusively utilizing photons and negating the wave aspect of optical duality.

After New Scientist covered their study, the team received significant interest from peers, with citations soaring. Villas-Boas shared, “I’ve received numerous invitations to present, including events in Japan, Spain, and Brazil,” emphasizing the widespread intrigue.

In the traditional double-slit experiment, an opaque barrier containing two narrow slits is positioned between a screen and a light source. Light travels through the slits to create a pattern of alternating bright and dark vertical stripes, known as classical interference, usually attributed to colliding light waves.

The researchers shifted away from this conventional explanation, examining the so-called dark state of photons—a unique quantum state that prevents interaction with other particles, hence not illuminating the screen. This perspective eliminates the necessity for light waves to clarify the observed dark stripes.

This reevaluation challenges a deeply ingrained view of light within quantum physics. Many educators expressed concern, with some remarking, “Your findings challenge the foundational concepts I’ve taught for years.” However, while some colleagues embraced the new perspective, others remained skeptically intrigued, following New Scientist‘s initial report.

Villas-Boas has been actively exploring implications surrounding the dark state of photons. His investigations revealed that thermal radiation, such as sunlight, can reside in a dark state, concealing a substantial portion of its energy due to a lack of interaction with other objects. Experimental validation could involve placing atoms in cavities where their interactions with light are meticulously examined, according to Villas-Boas.

His team’s reinterpretation of interference phenomena facilitates comprehension of previously perplexing occurrences, such as non-overlapping wave interactions. Moving beyond the wave model to incorporate distinct bright and dark photon states opens avenues for innovative applications. Villas-Boas envisions potential developments such as light-controlled switches and devices that selectively permit specific light types to pass.

In his view, all these explorations connect back to the essential principles of quantum physics, highlighting that engaging with quantum objects necessitates understanding their interactions with measurement devices—encompassing darkness itself. “This concept is intrinsic to quantum mechanics,” Villas-Boas asserts.

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Source: www.newscientist.com

Theobromine: A Dark Chocolate Compound That May Offer Anti-Aging Benefits

Researchers at King’s College London have found significant connections between theobromine, a widely-known plant compound from cocoa, and measures of epigenetic aging, indicating that theobromine may be associated with human aging.



third others. We illustrate that the documented beneficial relationship between health and aging and theobromine intake extends to the molecular epigenetic level in humans. Image credit: Sci.News.

“Coffee and cocoa are popular foods and are linked to lower rates of cardiovascular disease and mortality,” commented lead author Ramy Saad, Ph.D., along with colleagues.

“They contain several significant alkaloids, including theobromine, caffeine, theophylline, paraxanthine, and 7-methylxanthine.”

“Theobromine and 7-methylxanthine are partial metabolites of caffeine, yet both exist in much greater concentrations in cocoa as unprocessed primary metabolites.”

“Theobromine has long been associated with various health benefits and aging. For instance, studies in model organisms have confirmed a link between theobromine and extended lifespan.”

“Moreover, various human cohort observational studies have reported clear links between theobromine intake and multiple aspects of improved health.”

“Nonetheless, the exact impacts of theobromine on health and aging remain unclear, and the molecular pathways behind these effects are largely unknown.”

In the research, scientists analyzed the levels of theobromine in individuals’ blood against blood-based indicators of biological aging.

Across two European cohorts, which included 509 participants from TwinsUK and 1,160 from KORA, individuals with elevated levels of theobromine in their bloodstream exhibited a lower biological age compared to their chronological age.

“Our research discovered a correlation between key components in dark chocolate and prolonged youthfulness,” stated the study’s senior author, Professor Jordana Bell.

“While we’re not advocating for increased dark chocolate consumption, this study sheds light on how common foods might offer insights into healthier, longer living.”

The researchers also explored whether other metabolites found in cocoa and coffee reflected similar associations.

However, they concluded that the effect appears to be unique to theobromine.

Two different assessments were used to measure the biological age of participants.

Some researchers examined chemical alterations in DNA to estimate an individual’s aging rate.

Other scientists assessed the length of telomeres, the protective end caps of chromosomes, as telomere shortening is linked with aging and age-associated diseases.

“This is a fascinating finding, and the next crucial question is: What drives this association, and how can we further explore the interactions between dietary metabolites and the epigenome?” Dr. Saad remarked.

“This strategy could unveil significant discoveries about both common and rare diseases, as related to aging and beyond.”

“This study has uncovered another molecular mechanism through which natural compounds present in cocoa promote health,” noted study co-author Dr. Ricardo Costeira.

“Although further investigation is warranted, the findings highlight the importance of population-level analysis in the fields of aging and genetics.”

of findings Published in a journal on December 10th aging.

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Ramy Third others. Theobromine is associated with delayed epigenetic aging. aging published online on December 10, 2025. doi: 10.18632/aging.206344

Source: www.sci.news

Uncovering the Universe: Why We Just Recently Realized It’s Dark Instead of Bright

Adobe Stock Photo/Phoebe Watts

Set against the vastness of space, our blue planet emerges above the desolate lunar landscape. This iconic photograph, “Earthrise,” was captured by Apollo 8 astronaut Bill Anders on Christmas Eve 1968.

Nearly six decades later, we regard this image as part of our narrative. Yet, envision a different earthrise where space is not a dark backdrop, but a vivid blue, akin to a sunny sky. Odd as it may appear, this was the vision held by many Europeans for centuries.

Our comprehension of the cosmos has evolved significantly over time, influencing how we perceive our place within it. The shift from an earth-centered to a sun-centered universe, along with the transition from a finite to an infinite cosmos, prompted a profound reevaluation of humanity’s role in the grand scheme. The change from a vibrant to a dim universe is equally crucial, yet it remains largely overlooked in our historical narratives.

Recently, through my scholarly work in literary and scientific history, I have sought to trace the timeline of this transformation. At what point did our universe metaphorically turn dark? What did this shift imply for humanity?

Earthrise—a photograph from the moon’s surface in 1968 showcasing the notion that space is dark.

NASA

Reflect on the account given by Domingo González, the hero of Francis Godwin’s 1638 science fiction novel, The Man in the Moone. González travels to the moon in a swan-powered vehicle and notes a scarcity of stars. Even those he does see are dim. He observes, “It was always daytime for some reason, yet the stars appeared faint, similar to the moon’s glow in daylight.” Why are there fewer stars in his experience? Why do they appear washed out? Because, in his narrative, space is akin to the daytime sky, where the sun drowns out the luminosity of stars.

From our viewpoint, González’s reality seems inverted. In his portrayal, daytime reveals our true nature, while night conceals us within Earth’s shadow. Yet, ascending to space at midnight, we would eventually emerge from darkness into eternal daylight.

In Francis Godwin’s The Man in the Moone, protagonist Domingo González embarks for the moon in a swan-powered craft.

Houghton Library

While González omits mention of a shadow, we glimpse it in another early space narrative by John Milton, Paradise Lost. As Milton’s Satan nears Earth, he remarks upon “a whirling canopy / a spreading shadow of the night.” If you visualize pre-modern eras, adding this shadow to your image of earthrise transforms it. A dark cone emerges from the jagged globe, plunging into the azure sky and vanishing beneath the lunar horizon.

Additional authors elucidate why the Universe is imagined as not merely bright, but blue-hued. The prevalent rationale is that the “firmament” was envisioned as blue. Walter Charlton, a contemporary of Milton, remarked this notion was widely shared “by many transcendental thinkers, as well as the average populace.” Observing the daytime sky, they believed they were witnessing the universe’s limit.

The Path to Earthrise

This luminescent universe also manifests in visual art. A comparison with Apollo 8 is particularly pertinent. Hours after capturing earthrise, the crew transmitted radio messages from lunar orbit to Earth. Commander Frank Bowman extended Christmas wishes and recited the biblical creation tale. For the first time, humanity achieved a god-like vantage point of the radiant blue planet glistening against the abyss. In contrast, when pre-modern artists portrayed these scripture moments, they often rendered a dim planet against a bright celestial expanse. To reimagine earthrise, picture one of these shadowed Earths ascending above the lunar surface instead of the iconic “blue marble.”

It was not just poets and artists who envisioned such a realm. Philosophers and scientists also entertained the concept. Aristotle remarked on “the shadow of the earth (termed night).” Two millennia later, Copernicus similarly wrote, “While the rest of the universe is illuminated and radiant, the night signifies nothing but the shadow of the Earth, extending in a cone and culminating at a point.”

This perspective was not unreasonable; early European scholars lacked compelling evidence to argue otherwise, particularly concerning the light-refracting properties of the universe and Earth’s atmosphere. Without such evidence, why suspect that night predominates and day a rarity? What led pre-modern Christians to diverge from millennia of tradition and perceive heaven—not as eternal brightness, but infinite darkness?

A 13th-century manuscript depicting a gray Earth casting a black shadow against a blue universe (left) and a 15th-century manuscript showcasing the newly created Earth as a black marble surrounded by blue cosmos (right).

Heritage Image Partnership Ltd/Alamy; National Library of France

This does not imply that luminous spaces were universally accepted in pre-modern thought. For instance, scholars within the Islamic tradition favored the concept of dark spaces starting in the 9th century, yet this perspective seems to have been less influential in the West. In any case, the notion of a dark universe had to be re-established among 17th-century European thinkers.

During this period, significant advancements in atmospheric science emerged. Notably, the term “atmosphere” was coined in the 17th century, with Walter Charlton among the first to utilize it in English. His view of the universe acts as a transitional development in this narrative: a universe that oscillates between brightness and darkness based on an observer’s orientation towards the sun. Although Charlton described a dark universe, he noted that it was “not nearly as deep blue as many presume,” and filled with countless tiny particles or “atoms,” which he speculated could impact visibility. In contrast, Otto von Guericke, who endorsed the infinite universe and conducted pioneering vacuum experiments, postulated that in an “unblemished” and “void” space, devoid of illuminated objects, we would perceive “nothing but shadows.”

Thereafter, dark space gained traction among European scientists and thinkers informed by these scientific advancements. However, this marks only part of the narrative, as visions of bright spaces lingered in cultural imaginations for centuries.

Fast forward to 1858, when astronomer James Gall envisioned his foray into the void for a Victorian audience, exclaiming, “As I look around me, how peculiar! The heavens are pitch black.” While Gall acknowledged the darkness of space, he doubted the audience’s awareness of this fact. It wasn’t a naive child or uninformed individual believing in a “giant blue sphere,” but the renowned literary historian David Masson in 1880 who clung to this isolated imagery, which persisted well into the 1920s, right at the brink of the Space Age.

Thus, we confront a dual narrative of a decline in our cosmic imagination alongside the unexpected evolution of these ideas. Some of the most striking evidence is found in literature, especially in space travel narratives, which were initially recognized by literary scholars such as C.S. Lewis and more recently John Leonard. Nevertheless, this aspect has yet to receive thorough investigation, and its cultural ramifications remain largely unexamined.

The implications are significant, often concealed in plain sight. Prominent images such as earthrise have reshaped our perceptions of our planet and its environmental context. The view of Earth as “perfect” and “blue” has also rendered it “fragile,” symbolizing the perils of nuclear conflict and climate change, as well as underscoring the call for political unity and ecological stewardship. What is less acknowledged, however, is that this transformation arose not only from a fresh perspective on Earth, but importantly on the vastness surrounding it.

For millennia, the entirety of Earth has been envisioned, represented, and contemplated. Yet, much of it was depicted within brilliant space, eliciting markedly different responses. Hence, the influence of earthrise was indeed more profound than commonly appreciated. The mass circulation of such imagery has obliterated even the faintest remnants of a once-bright universe and firmly imprinted its inversion into collective consciousness. The Earth stands not merely as “blue” or “fragile.” While it may appear thus against the cold, dark expanse surrounding it, it has transitioned into both a scientific reality and a cultural perception.

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Supermassive Dark Matter Stars Could Be Hidden in the Early Universe

Exotic stars may be fueled by dark matter

remote vfx/getty images

We might be observing the earliest indications of peculiar stars that harness dark matter. These dark stars could provide explanations for some of the universe’s most enigmatic entities, and offer insights into the actual nature of dark matter itself.

Standard stars are birthed when a gas cloud collapses, leading to a core dense enough to initiate nuclear fusion. This fusion generates significant heat and energy, radiating into the surrounding gas and plasma.

Dark stars could have emerged in a similar fashion during the universe’s infancy, a period of higher density which also saw a notably concentrated presence of dark matter. If a gas cloud collapsing into a star contains substantial dark matter, it may begin to collide and dissipate prior to nuclear fusion, generating enough energy to illuminate the dark star and halt further collapse.

The process leading to the formation of dark stars is relatively straightforward, and currently, a team led by Katherine Freese from the University of Texas at Austin is exploring its potential outcome.

In an ordinary large star, once the hydrogen and helium are depleted, it continues fusing heavier elements until it runs out of energy and collapses into a black hole. The more mass the star contains, the quicker this transition occurs.

However, the same is not true for dark stars. “By incorporating dark matter into a star roughly the mass of the Sun, and sustaining it through dark matter decay rather than nuclear means, you can continuously nourish the star. Provided it receives enough dark matter, it won’t undergo the nuclear transformations that lead to complications,” explains George Fuller, a collaborator with Freese at the University of California, San Diego.

Despite this, general relativity imposes a limit on how long dark matter can preserve these unusual giants. Albert Einstein’s theory suggests that an object’s gravitational field does not increase linearly with mass; instead, gravity intensifies the gravitational force. Ultimately, an object may reach a mass at which it becomes unstable, with minor variations overpowering its gravitational pull and resulting in a collapse into a black hole. Researchers estimate this threshold for a dark star is between 1,000 and 10 million times the Sun’s mass.

This mass range makes supermassive dark stars prime candidates for addressing one of the early universe’s profound mysteries: the existence of supermassive black holes. These giants were spotted relatively early in the universe’s history, but their rapid formation remains a puzzle. One prevailing theory posits that they didn’t arise from typical stars, but rather from some colossal “seed.”

“If a black hole weighs 100 solar masses, how could it possibly grow to a billion solar masses in just a few hundred million years? This is implausible if black holes were formed solely from standard stars,” asserts Freese. “Conversely, this situation changes significantly if the origin is a relatively large seed.” Such faint stars could serve as those seeds.

Yet, the enigmas of the early universe extend beyond supermassive black holes that dark stars could elucidate. The James Webb Space Telescope (JWST) has unveiled two other unforeseen object types, referred to as the little red dot and the blue monster, both appearing at substantial distances. The immediate hypothesis for these is that they are compact galaxies.

However, like supermassive black holes, these objects exist too far away and too early in universal history for simple formation explanations. Based on observations, Freese and her associates propose that both the little red dot and the blue monster may represent individual, immensely massive dark stars.

If they indeed are dark stars, they would display particular clues in their light. This aspect pertains to specific wavelengths that dark stars should ostensibly absorb. Normal stars and galaxies dense with them are too hot to capture that light.

Freese and colleagues have found possible indicators of this absorption in initial JWST observations of several distant entities; however, the data is too inconclusive to confirm its existence. “Currently, of all our candidates, two could potentially fit the spectrum: a solitary supermassive dark star or an entire galaxy of regular stars,” Freese notes. “Examining this dip in the spectrum, we’re convinced it points to a dark star rather than a conventional star-filled galaxy. But for now, we only possess a faint hint.”

While it remains uncertain if we have definitively detected a dark star, this development marks progress. “It isn’t a definitive finding, but it certainly fuels motivation for ongoing inquiries, and some aspects of what JWST has been examining seem to align with that direction,” remarks Dan Hooper from the University of Wisconsin-Madison.

Establishing whether these entities are genuinely dark stars necessitates numerous more observations, ideally with enhanced sensitivity; however, it remains ambiguous whether JWST can achieve the level of detail required for such distant galaxies or dark stars.

“Confirming the existence of dark stars would be a remarkable breakthrough,” emphasizes Volodymyr Takistov from the High Energy Accelerator Research Organization in Japan. This could facilitate new observational avenues into foundational physics. This is particularly true if dark stars are recognized as seeds for supermassive black holes. Freese, Fuller, and their team deduced that the mass at which a black hole collapses correlates with the mass of the dark matter particle annihilating at its center, implying that supermassive black holes could serve as metrics to evaluate or at least restrict dark matter properties. Of course, validating the existence of dark stars is the first priority. “Even if these entities exist, their occurrence is rare,” Hooper states. “They are uncommon, yet significant.”

Exploring the Mysteries of the Universe: Cheshire, England

Join some of the brightest minds in science for a weekend dedicated to unraveling the universe’s mysteries, featuring a tour of the legendary Lovell Telescope.

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Why Dark Matter Is Still One of Science’s Greatest Mysteries

“As we approach the late 2020s, it is an incredibly exciting era for dark matter research…”

Sackmestelke/Science Photo Library

This is an extraordinary moment for dark matter researchers. Despite cuts in funding from governments globally, dark matter continues to represent one of the most captivating and significant unsolved mysteries in physics and in the broader scientific landscape. The majority of matter in the universe seems invisible. For every kilogram of visible matter, there are approximately five kilograms of dark matter. This is inferred from the gravitational influence dark matter exerts on the structures of visible components in the universe.

Galaxy clusters are most effectively explained when considering dark matter as a component. Observations of the distribution of the earliest light in the universe fit theoretical predictions only by including dark matter in the model. Many other observations similarly support this view. Dark matter is abundant and remains undetectable unless we study its effects on normal matter.

As we enter the late 2020s, it’s a thrilling period for dark matter research. Investigations by the European Space Agency’s Euclid Space Telescope promise to deepen our understanding of galactic structures. Simultaneously, the Vera C. Rubin Observatory has commenced a decade-long sky survey that is likely to transform our comprehension of satellite galaxies orbiting larger galaxies. These dynamics enhance our understanding of how dark matter influences visible matter.

Exploring phenomena we know exist yet cannot observe directly challenges our creativity as scientists. Some of the pivotal questions that we must ponder include: Can we trap dark matter particles in a laboratory setting? If not, what methods can we employ to analyze their properties?

The solution lies in progressing from established knowledge. We suspect that dark matter behaves similarly to known matter, indicating we might utilize the same mathematical frameworks, like quantum field theory (QFT), to investigate it.


We are increasingly focusing on finding evidence of dark matter scatterings, not just impacts on targets.

Quantum field theory can seem complex, and indeed it is. However, a deep understanding is not mandatory to grasp its essence. It is potentially the most fundamental physical theory, harmonizing special relativity with quantum mechanics (excluding general relativity). It suggests that interactions at any point in the universe might give rise to particles due to respective fields.

Imagine a strawberry field. Strawberries grow in specific places due to certain characteristics of those space-time coordinates. These areas possess conditions suitable for strawberry flowers to flourish. The potential for strawberries exists throughout the field, yet only select areas yield blossoms. Similarly, QFT posits the existence of particles.

QFT is intricate, a realm where even experts invest years to cultivate understanding. Even when considering the application of QFT to dark matter to glean useful insights, a critical question arises: How can one formulate an equation for something with minimal known properties?

Sociologically, it’s fascinating to observe the varied responses from scientists. Over the past decade, a popular method for addressing what remains unknown has involved crafting “effective field theory” (EFT). EFT enables the formulation of generalized equations that can be adapted based on empirical observations.

EFT can also be designed with specific experimental frameworks in mind. A key strategy for unraveling dark matter mysteries involves conducting direct detection experiments. Through these efforts, we aspire to witness interactions between dark and visible matter that yield observable results in ground-based studies. Over the years, methods of direct detection have matured and diversified. Researchers are not only looking for signs of dark matter striking targets; they are increasingly seeking footprints of dark matter scattering from electrons. This shift requires an evolution of EFT to accommodate new experimental insights.

In a recent preprint, researchers Pierce Giffin, Benjamin Lillard, Pankaj Munbodh, and Tien-Tien Yu present an EFT aimed at better addressing these scattering interactions. This paper, which has not yet undergone peer review, captured my attention as a prime example of research that may not make headlines but represents essential progress. Science demands patience, and I trust our leaders will remain cognizant of that.

Chanda Prescod-Weinstein is an associate professor of physics and astronomy at the University of New Hampshire. She is the author of Turbulent Universe and upcoming books The Ends of Space and Time: Particles, Poetry, and the Boogie of Cosmic Dreams.

What I Am Reading
I just completed the captivating debut novel by Addie E. Sitchens: Dominion.

What I See
I recently caught up on the summer episodes of Emmerdale, and they were quite surprising!

What I Am Working On
My collaborators and I are exploring intriguing new research ideas related to dark matter scenarios.

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Lava Tubes Hold Secrets of Unidentified ‘Microbial Dark Matter’ – Sciworthy

Mars’ surface is not currently conducive to human life. It presents extreme challenges, including a tenuous atmosphere, freezing temperatures, and heightened radiation levels. While Earth’s extremophiles can tackle some obstacles, they can’t handle them all simultaneously. If Martian life exists, how do these microbes manage to survive in such an environment?

The answer might lie within caves. Many researchers believe that ancient lava tubes on Mars formed billions of years ago when the planet was warmer and had liquid water. Caves serve as shelters against radiation and severe temperatures found on the Martian surface. They also host the nutrients and minerals necessary for sustaining life. Although scientists cannot yet explore Martian caves directly, they are examining analogous sites on Earth to establish parameters for searching for life on Mars.

A research team, led by C.B. Fishman from Georgetown University, investigated the microorganisms inhabiting the lava tubes of Mauna Loa, Hawaii, to learn about their survival mechanisms. Thanks to careful conservation efforts by Native Hawaiians, these lava tubes remain undisturbed by human activity. Researchers believe that both the rock structures in Mauna Loa Cave and the minerals formed from sulfur-rich gases bear similarities to Martian cave formations.

The team analyzed five samples from well-lit areas near the cave entrance, two from dimly lit zones with natural openings known as skylights, and five from the cave’s darkest recesses. Samples were chosen based on rock characteristics, including secondary minerals like calcite and gypsum, and primary iron-bearing minerals such as olivine and hematite.

Findings revealed significant variation in mineralogy within the cave, even over small distances. The bright samples were predominantly gypsum, while the dark samples lacked these key minerals. Instead, one dark sample was rich in iron-bearing minerals, while another contained mainly calcite, gypsum, and thenardite.

To identify the microorganisms within the samples, the team employed the 16S rRNA gene to recognize known microbes and understand their relationships. They also reconstructed complete genomes from cave samples using a method called metagenomic analysis. This technique is akin to following instructions to assemble various models from mixed DNA fragments. Such insights help researchers grasp how both known and unknown microorganisms thrive in their respective environments.

The team discovered that approximately 15% of the microbial genomes were unique to specific locations, with about 57% appearing in less than a quarter of the samples. Furthermore, microbial communities in dark regions exhibited less diversity and were more specialized compared to those in well-lit areas. While dark sites were not as varied as bright ones, each supported its own distinct microbial community.

To explain this difference, the researchers proposed that dark microbes have limited survival strategies since photosynthesis is impossible without light. Instead, these microbes extract chemical energy from rocks and decaying organic matter, much like how humans derive energy from breaking down food.

The findings from metagenomic data indicated that even though sulfur minerals were abundant, very few microorganisms specialized in sulfur consumption were present. This aligns with expectations in oxygen-rich environments, as oxygen tends to react with sulfur, making it unavailable to microorganisms. The researchers suggested that sulfur-metabolizing microbes may be more commonly found in low-oxygen environments, such as Mars.

Additionally, the study revealed that a majority of the microorganisms found in these caves were previously undescribed by science, contributing to what is referred to as microbial dark matter. The existence of such unknown microorganisms hints at novel survival strategies.

The research team concluded that lava tube caves could be a crucial source of new microorganisms, aiding astrobiologists in their quest to understand potential life forms on Mars. They recommended that future investigations into Martian caves should focus on detecting small-scale microbes in various mineral contexts. Over time, the interplay between cave conditions and Martian microorganisms may be unveiled as Mars becomes less habitable.


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Source: sciworthy.com

Potential First Signs of Dark Matter Discovered

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Unexplained radiation surrounding the Milky Way may hint at dark matter’s composition

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A mysterious glow detected in the outer regions of the Milky Way may provide the first clues about the nature of dark matter, yet astronomers caution that it’s premature to draw any definitive conclusions.

Dark matter is theorized to account for 85% of the universe’s total mass, but scientists have struggled to identify the particles constituting it.

Among the potential candidates for dark matter are weakly interacting massive particles (WIMPs). These elusive particles are notoriously hard to detect as they seldom interact with normal matter but are believed to occasionally self-annihilate, creating bursts of high-energy radiation in the form of gamma rays.

If dark matter is uniformly distributed across the galaxy as indicated by its gravitational effects, and if it consists of WIMPs, we should observe gamma rays as these particles self-annihilate. For over a decade, astronomers have been investigating whether the anomalously high gamma-ray emissions from the galactic center could signal this phenomenon, yet conclusive evidence remains elusive.

Now, Tomonori Toya, a professor at the University of Tokyo, claims he may have detected such a signal emanating from the Milky Way’s outer halo, utilizing 15 years’ worth of observations from NASA’s Fermi Gamma-ray Space Telescope.

Toya devised a model predicting the expected gamma-ray radiation in this region based on established sources like stars, cosmic rays, and vast bubbles of radiation identified above and below the Milky Way. Upon subtracting this known radiation from the total observed by Fermi, he found a residual gamma-ray glow with an energy level around 20 gigaelectronvolts.

This specific gamma-ray energy strongly aligns with the theoretically anticipated emissions from WIMPs’ self-annihilation, according to Toya. Although he admits it is too early to assert that these gamma-ray spikes are definitively due to dark matter, he describes the findings as “the most promising candidate for radiation from dark matter known to date.”

“Though the research began with the aim of identifying dark matter signals, I initially felt skeptical—like winning the lottery. When I first observed what seemed to be a signal, I approached it with caution,” says Totoni. “However, after thoroughly checking everything and confirming its accuracy, I was filled with excitement.”

“This represents a significant result worthy of further investigation, but firm conclusions cannot be drawn at this stage,” states Francesca Karoly from the French National Center for Scientific Research in Annecy. Accurately modeling all gamma-ray sources in the Milky Way, aside from dark matter, is quite complex, and Totoni has yet to deeply validate her models.

Silvia Manconi of France’s Sorbonne University asserts that the results need additional scrutiny, and more robust models are essential to establish whether the signals are genuine. Additionally, gamma-ray signals from other sources, like dwarf galaxies, are still unobserved and require thorough explanation, she mentions.

Many alternative radiation sources, including radio waves and neutrinos, will also need analysis to ensure the gamma rays aren’t being attributed to something else, says Anthony Brown from Durham University, UK. “Analyzing from just one perspective isn’t sufficient,” he states. “Dark matter necessitates an abundance of high-quality data.”

CERN and Mont Blanc: Exploring dark matter and frozen phenomena in Switzerland and France

Get ready to experience the wonders of CERN, the European center for particle physics, situated near the picturesque city of Geneva, where scientists operate the renowned Large Hadron Collider.

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Mysterious Glow Around the Milky Way May Provide First Evidence of Dark Matter

For nearly a century, dark matter has posed a significant enigma. Although it outnumbers ordinary matter by a ratio of five to one, it remains invisible and undetectable by current technology.

A daring new analysis of 15 years of data from NASA’s Fermi Gamma-ray Space Telescope now claims to shed light on this mystery.

The latest research reveals the detection of a peculiar halo-like glow of gamma rays surrounding the Milky Way galaxy, with distinct peaks in energy that align closely with the signals predicted for a specific type of hypothetical dark matter particle.

These particles, referred to as weakly interacting massive particles (WIMPs), can generate gamma rays by annihilating one another.

“If this is validated, it would be the first instance where humanity has ‘seen’ dark matter,” stated Professor Tomonori Toya, an astronomer at the University of Tokyo and co-author of the study.

In an interview with BBC Science Focus, he expressed his initial skepticism: “When I first noticed what looked like a traffic light, I was doubtful, but after careful investigation, I became convinced it was accurate—it was an exhilarating moment,” he shared.

However, despite the excitement surrounding the new signals, independent experts caution that this discovery is far from conclusive.

This possible breakthrough emerges nearly a century after Swiss astronomer Fritz Zwicky first proposed dark matter’s existence, after observing that the galaxies in the Milky Way cluster were moving too swiftly for their visible mass.

Mr. Toya’s study, published in the Journal of Cosmology and Astroparticle Physics, scrutinized 15 years of data from the Fermi telescope, focusing on the regions above and below the Milky Way’s main disk—known as the galactic halo.

After modeling and accounting for known sources of gamma rays, such as interstellar gas interactions, cosmic rays, and massive bubbles of high-energy plasma at the galaxy’s center, he identified a leftover component that shouldn’t exist.

“We detected gamma rays with a photon energy measuring 20 giga-electron volts (or an impressive 20 billion electron volts), extending in a halo-like formation toward the Milky Way’s center,” Toya explained. “This gamma-ray-emitting component aligns with the expected shape of a dark matter halo.”

A gigaelectronvolt (GeV) represents a unit of energy utilized by physicists to quantify subatomic particles’ energy levels—approximately a billion times the energy that a single electron attains when traversing a 1-volt battery.

The potential dark matter signal identified by Toya sharply rises from a few GeV, peaks around 20 GeV, and subsequently declines, consistent with predictions for WIMPs, which possess about 500 times the mass of a proton.

This gamma-ray intensity map illustrates a signal that may originate from dark matter encircling the Milky Way halo. The gray horizontal bar in the central area represents the galactic plane, which was exempted from the analysis to avoid strong astrophysical radiation. – Photo credit: Tomonori Toya, University of Tokyo

In Totani’s perspective, this data significantly indicates the existence of dark matter. “This marks a crucial advancement in astronomy and physics,” he asserts.

Nevertheless, Jan Conrad, a professor of astroparticle physics at Stockholm University in Sweden and an independent expert in gamma-ray searches for dark matter, advises prudence.

“Making claims based on Fermi data is notoriously challenging,” he remarked to BBC Science Focus.

This isn’t the first instance of astronomers witnessing such phenomena; the story stretches back to 2009, shortly after the Fermi telescope’s launch. In that year, researchers identified an unexplained surplus of gamma rays emanating from the galactic center.

For years, this finding stood out as a compelling hint of dark matter. However, Conrad pointed out that even after 16 years, the scientific community has yet to arrive at a consensus about the signal’s dark matter roots.

“It’s believed to be related to dark matter,” he claims. “Despite accumulating data and enhanced methods since then, the question of dark matter’s existence remains unresolved.”

Even at this juncture, researchers who have spent over a decade working to disprove the galactic center excess are unable to definitively prove it is astrophysical in nature (originating from sources other than dark matter), nor can they confirm it is attributable to dark matter. The issue remains unsolved.

Conrad emphasized that the emerging signals from the halo are insufficiently studied and will likely necessitate many more years of investigation for verification. Both the new halo anomaly and the much-debated galactic center signal share a common challenge: noise interference.

In these regions, gamma rays potentially stemming from dark matter annihilation may also originate from numerous other, poorly understood sources—complicating efforts to reach definitive conclusions.

“The uncertainties surrounding astrophysical sources make it exceedingly difficult to assert strong claims,” Conrad stated.

Despite their differing confidence levels, both Totani and Conrad highlight the same forthcoming focus: dwarf galaxies.

These small, faint galaxies orbiting the Milky Way are believed to contain significant amounts of dark matter while exhibiting minimal astrophysical gamma-ray background, rendering them ideal for studying dark matter annihilation.

“If we detect a similar excess in dwarf galaxies, that would provide compelling evidence,” Conrad said. “Dwarf galaxies provide a much cleaner environment, allowing for potential confirmation.”

Dr. Toya concurred, noting, “If the results of this study are validated, it wouldn’t be surprising to observe gamma rays emitting from dwarf galaxies.”

The Cherenkov Telescope Array Observatory (CTAO) is the most sensitive ground-based gamma-ray observatory ever constructed, offering a powerful new approach to scrutinize whether this enigmatic signal is indeed dark matter. – Photo credit: Getty

Yet, the ultimate verification of Toya’s discovery might be closer to home. Experiments designed to detect dark matter are currently taking place in facilities situated deep underground around the world.

“If we were to observe a signal there that aligns with a WIMP of the same mass…that would present a robust argument, as it would be much cleaner,” Conrad pointed out.

In the coming years, the next-generation Cherenkov Telescope Array Observatory (CTAO) will significantly enhance sensitivity to high-energy gamma rays, enabling researchers to analyze halo signals with greater detail.

“Naturally, if this turns out to be true, it’s a significant discovery,” Conrad said. “The true nature of dark matter remains elusive. A clear signal indicating dark matter particles would be monumental. However, further research is essential to explore alternative explanations for this excess.”

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Scientists Have Studied Dark Matter for Decades—One May Have Caught a Glimpse.

Few entities in the universe are as intricate as dark matter, an unseen and exotic “matter” believed to account for most of the mass within galaxies.

The hypothesis suggests that aligning our current physical theories with observed universe phenomena necessitates the presence of substantial volumes of invisible matter. Scientists are convinced that this “missing mass” is real due to its gravitational pull, although direct detection has eluded them; they can only infer its presence.

Nearly a century after dark matter was first hypothesized, Japanese astrophysicists claim to have found the first concrete evidence of its existence—gamma rays emanating in a halo-like formation near the heart of the Milky Way.

“Naturally, we’re extremely enthusiastic!” said Tomonori Toya, a professor in the astronomy department at the University of Tokyo, in an email to NBC News. “While the research aimed at detecting dark matter, I thought the chances of success felt akin to hitting the jackpot.”

Toya’s assertion of being the first to identify dark matter is met with skepticism by some experts. Nonetheless, the findings, published on Tuesday in the Journal of Cosmology and Astroparticle Physics, shed light on the relentless pursuit of dark matter and the challenges of investigating the unseen in space.

Dark matter is estimated to constitute around 27% of the universe, whereas ordinary matter (like humans, objects, stars, and planets) makes up roughly 5%, according to NASA. The remainder consists of another enigmatic component known as dark energy.

Toya’s research utilized data from NASA’s Fermi Gamma-ray Space Telescope, which is focused on the center of our galaxy. This telescope is adept at capturing a powerful form of electromagnetic radiation called gamma rays.

The idea of dark matter was first proposed by Swiss astronomer Fritz Zwicky in the 1930s when he detected anomalies in the mass and movement of galaxies within the gigantic Coma cluster. The galaxies’ velocities exceeded expectations, implying they were bound together rather than escaping the cluster.

The subsequent theory introduced a truly extraordinary form of matter. Dark matter is undetectable because it does not emit, absorb, or reflect light. However, given its theoretical mass and spatial occupation in the universe, its presence can be inferred from its gravitational effects.

Various models strive to elucidate dark matter, but scientists contend that it comprises exotic particles that exhibit different behaviors compared to familiar matter.

One widely considered theory posits that dark matter consists of hypothetical particles known as WIMPs (weakly interacting massive particles), which have minimal interaction with ordinary matter. However, when two WIMPs collide, they can annihilate and emit potent gamma rays.

In his investigation, Toya identified a gamma-ray emission equating to about one millionth of the brightness of the Milky Way. The gamma rays also appeared spread out in a halo-like formation across extensive sky areas. Should these emissions originate from a single source, it may indicate that black holes, stars, or other cosmic entities, rather than diffuse dark matter, generate the gamma rays.

Gamma-ray intensity map covering roughly 100 degrees toward the galactic center. The gray horizontal line in the central section corresponds to the galactic plane, which was excluded from the analysis to avoid strong astrophysical radiation.Tomonori Toya / University of Tokyo

“To my knowledge, there’s no cosmic phenomena that would cause radiation exhibiting the spherical symmetry and unique energy spectrum observed here,” Toya remarked.

However, certain scientists not associated with the study expressed doubts about the findings.

David Kaplan, a physics and astronomy professor at Johns Hopkins University, emphasized that our understanding of gamma rays is still incomplete, complicating efforts to reliably connect their emissions to dark matter particles.

“We don’t yet know all the forms of matter in the universe capable of generating gamma rays,” Kaplan indicated, adding that these high-energy emissions could also originate from rapidly spinning neutron stars or black holes that consume regular matter and emit energetic jets.

Thus, even when unusual gamma-ray emissions are identified, deriving meaningful interpretations is challenging, noted Eric Charles, a scientist at Stanford University’s SLAC National Accelerator Laboratory.

“There are numerous intricacies we don’t fully grasp, and we observe a plethora of gamma rays across extensive areas of the sky linked with galaxies. It’s particularly difficult to decipher what transpired there,” he explained.

Dillon Braut, an assistant professor at Boston University’s Department of Astronomy and Physics, remarked that the gamma-ray signals and halo-like formations discussed in the study appear in regions of the sky that are “incredibly challenging to model.”

“Therefore, any claims should be treated with utmost caution,” Braut communicated to NBC News via email. “And, naturally, extraordinary claims necessitate extraordinary proof.”

Kaplan labeled the study as “intriguing” and “meriting further investigation,” but remained uncertain if subsequent analyses would substantiate the findings. Nonetheless, he anticipates that future advancements will allow scientists to directly validate dark matter’s existence.

“It would be a monumental shift as it appears poised to dominantly influence the universe,” he stated. “It accounts for the evolution of galaxies and, consequently, stars, planets, us, and is crucial for comprehending the universe’s origin.”

Toya himself acknowledged that further exploration is necessary to authenticate or refute his assertions.

“If accurate, the outcomes would have such significance that the research community would earnestly evaluate their legitimacy,” he noted. “While I have confidence in my findings, I hope other independent scholars can verify these results.”

Source: www.nbcnews.com

Green Bank Telescope Maps Cold ‘Dark’ Gas in Cygnus X

An astronomer utilizing the Green Bank Telescope (GBT) has developed an extensive map of carbon monoxide (CO) and dark molecular gas in star-forming complexes, particularly in Cygnus X.



These images illustrate the location of CO-dark molecular gas within Cygnus X. Image credit: NSF/AUI/NSF’s NRAO/P.Vosteen.

For decades, scientists have recognized that most new stars are birthed in frigid clouds of molecular hydrogen gas.

A significant portion of this molecular hydrogen remains elusive to most telescopes as it fails to emit easily detectable light.

Astronomers have typically sought these clouds by examining carbon monoxide (CO), a molecule that serves as a glowing signal for star-forming regions.

However, it has been uncovered that CO houses a considerable amount of “non-glowing” gas conducive to star formation.

This concealed material, referred to as CO-dark molecular gas, has represented one of astronomy’s most significant blind spots.

In a fresh study, NRAO astronomer Kimberly Emig and her team mapped this hidden gas across extensive sections of the sky, using radio spectral lines from atomic recombination known as carbon radio recombination lines (CRRLs).

Their map encompasses Cygnus X, a star-forming region located approximately 5,000 light-years away in the constellation Cygnus.

“It’s akin to suddenly switching on a light in a room and discovering various structures that were previously unseen,” Dr. Emig remarked.

The newly constructed map unveils a sprawling network of arcs, ridges, and webs of dark gas permeating Cygnus X.

These formations indicate where star-forming materials accumulate and evolve before becoming noticeable as molecular clouds in CO.

The authors demonstrated that these faint carbon signals, observed at very low radio frequencies, serve as an extraordinarily powerful instrument for uncovering hidden gas that directly correlates ordinary matter with the birth of new stars.

They found that this dark gas is not static; instead, it flows, shifts, and moves at rates much faster than previously recognized. These dynamics influence the stellar formation rate.

Moreover, they discovered that the intensity of these carbon lines is directly connected to the intense starlight bathing the area, emphasizing the significant role radiation plays in galactic recycling.

“By illuminating the invisible, we can trace how the raw ingredients in our galaxy transform from simple atoms into complex molecular structures that will ultimately become stars, planets, and potentially life,” Dr. Emig stated.

“This marks merely the beginning of comprehending an otherwise unseen force.”

Find the results published in the October 17th edition of the Astrophysical Journal.

_____

Kimberly L. Emig et al. 2025. The cold dark gas of Cygnus X: the first large-scale mapping of low-frequency carbon recombination lines. APJ 992, 216; doi: 10.3847/1538-4357/adfa17

Source: www.sci.news

Could the Internet Go Dark? Exploring the Vulnerable Systems That Connect Our Modern World

Waking up to a world without internet might seem liberating, but you may find yourself pondering your next steps.

If you have a checkbook handy, consider using it to purchase some groceries. Should your landline still function, you can reach out to your employer. Then, as long as you still remember how to find your way without modern navigation, a trip to the store is possible.

The recent outage in a Virginia data center highlighted that while the internet is a crucial component of contemporary existence, its foundation rests on aging systems and physical components, leading many to question what it would take for it to come crashing down.

The answer is straightforward: a streak of bad luck, deliberate cyberattacks, or a combination of both. Severe weather events can knock out numerous data centers. Unexpected triggers in AI-generated codes at significant providers like Amazon, Google, and Microsoft could lead to widespread software failures. Armed interventions targeting critical infrastructure could also play a role.

Although these scenarios would be devastating, the more significant concerns for a select group of internet specialists revolve around sudden failures in the outdated protocols that support the entire network. Picture this as a plumbing system that manages connection flows or an address directory that allows machines to locate one another.

We refer to it as “the big one,” but if that occurs, having a checkbook on hand might be crucial.

Something substantial could commence When a tornado swept through Council Bluffs, Iowa, it ravaged a set of low-lying data centers critical to Google’s operations.

This region is known as us-central1, one of Google’s data center clusters, vital for various services including its cloud platform, YouTube, and Gmail (2019) power outages reported here took place that affected users across the United States and Europe.

As YouTube cooking videos become glitchy, dinner preparations go awry. Employees worldwide rush to update emails that suddenly vanish, resorting to face-to-face communication instead. US officials noted a deterioration in certain government services before refocusing their efforts on a new operation against Signal.

While this situation is inconvenient, it doesn’t signify the end of the internet. “Technically, as long as two devices are connected with a router, the Internet functions,” states Michał “Risiek” Wojniak, who works in DNS, the system linked to this week’s outage.

However, “there’s a significant concentration of control happening online,” points out Stephen Murdoch, a computer science professor at University College London. “This mirrors trends in economics: it’s typically more cost-effective to centralize operations.”

But what if extreme heat wipes out US East-1, part of the Virginia facility housing “Data Center Array,” a crucial node for Amazon Web Services (AWS), the epicenter of this week’s outage, as well as nearby regions? Meanwhile, a significant cluster in Europe suffers a cyberattack. frankfurt or London. As a result, the network may redirect traffic to a secondary hub (a less-frequented data center), which subsequently faces capacity issues akin to a congested side road in Los Angeles.

Aerial view of the Amazon Web Services data center known as US East-1 in Ashburn, Virginia. Photo: Jonathan Ernst/Reuters

Alternatively, if we shift focus from disaster scenarios to automation risks, increased traffic might unveil hidden bugs within AWS’s internally revised infrastructure, possibly an oversight from months prior. Earlier this summer, two AWS employees were let go amid a broader push towards automation. Faced with an influx of unknown requests, AWS begins to falter.

The signal will falter, and so will Slack, Netflix, and Lloyds Bank. Your Roomba vacuum becomes silent. Smart mattresses may misbehave, just like smart locks.

Without Amazon and Google, the internet would be nearly unrecognizable. Together, AWS, Microsoft, and Google command over 60% of the global cloud services market, making it nearly impossible to quantify the number of services reliant on them.

“However, at its core, the Internet continues to operate,” remarks Doug Madley, an expert in internet infrastructure who studies disruptions. “While the usual activities may be limited, the underlying network remains functional.”

You might believe the biggest risk lies in attacks on undersea cables. While this notion captivates think tanks in Washington, little action has materialized. Undersea cables incur regular damage, Madley notes, with the United Nations estimating between 150 to 200 faults occurring annually.

“To significantly impair communication, a vast amount of data must be disrupted. The undersea cable sector often asserts, ‘We manage these issues routinely.’

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Subsequently, a group of anonymous hackers targets a DNS service provider, a key player in the Internet’s directory system. For example, Verisign manages all online domains ending with certain “.com” or “.net” suffixes. Other providers oversee domains like “.biz” and “.us.”

According to Madley, the likelihood of such a provider being taken down is minimal. “If anything were to happen to VeriSign, .com would vanish, which presents a strong financial motivation for them to prevent that.”

Collectively, AWS, Microsoft, and Google dominate over 60% of the global cloud services market. Photo: Sebastian Boson/AFP/Getty Images

To genuinely disrupt the larger ecosystem, a colossal error involving fundamental infrastructure beyond Amazon or Google would be required. Such a scenario would be unprecedented; the closest parallel occurred in 2016 when an attack on Dyn, a small DNS provider, brought down Guardian, X, among others.

If .com were to disappear, essential services like banks, hospitals, and various communication platforms would vanish too. Although some elements of the government’s internet structure remain intact, such as the U.S. secure messaging system Siprnet.

Yet, the internet would persist, at least for niche communities. There are self-hosted blogs, decentralized social networks like Mastodon, and particular domains like “.io” or “.is.”

Murdoch and Madrid contemplate a drastic scenario capable of eliminating the rest. Murdoch alludes to a potential bug in the BIND software supporting DNS. Meanwhile, Madrid emphasizes testimonies from Massachusetts hackers who informed Congress in 1998 about a vulnerability that could “bring the Internet down in 30 minutes.”

This vulnerability pertains to a system one layer above DNS: the Border Gateway Protocol, directing all web traffic. Madley argues that such an event is highly improbable, as it would require a full-scale emergency response, and the protocols are “incredibly resilient; otherwise, we would have already experienced a collapse.”

Even if the internet were to be entirely shut down, it’s uncertain whether it would ever reboot, warns Murdoch. “Once the Internet is active, it doesn’t get turned off. The method of restarting it is not well understood.”

The UK previously had a contingency plan for such a situation. Should the internet ever be disabled, Murdoch notes, individuals knowledgeable about its workings would gather at a pub outside London and brainstorm the next steps.

“I’m not sure if this is still true. This was years ago, and I couldn’t recall the exact pub.”

Source: www.theguardian.com

Study Reveals Disappearance of Dark Matter as Cause for Excess Galactic Centers in the Milky Way

The galactic center excess refers to an unexpected intensity of gamma rays emerging from the core of the Milky Way galaxy.



This view displays the entire sky at energies exceeding 1 GeV, derived from five years of data from the LAT instrument on NASA’s Fermi Gamma-ray Space Telescope. The most striking aspect is a luminous band of diffuse light along the center of the map, indicating the central plane of the Milky Way galaxy. Image credit: NASA/DOE/Fermi LAT collaboration.

Gamma rays are a form of electromagnetic radiation characterized by the shortest wavelengths and the highest energy.

The intriguing gamma-ray signal from the Milky Way’s center was initially observed in 2009 by the Large Area Telescope, the primary instrument of NASA’s Fermi Gamma-ray Space Telescope.

The source of this signal remains under discussion, with main hypotheses involving self-annihilating dark matter and undetected populations of millisecond pulsars.

“When Fermi directed its gaze toward the galaxy’s center, the outcome was unexpected,” remarked Dr. Noam Libeskind, an astrophysicist at the Leibniz Institute for Astrophysics in Potsdam.

“The telescope detected an excessive number of gamma rays, the most energetic form of light in the universe.”

“Astronomers worldwide were baffled, and numerous competing theories emerged to clarify the so-called gamma-ray excess.”

“After extensive discussion, two primary theories surfaced: either these gamma rays stem from millisecond pulsars (highly dense neutron stars rotating thousands of times per second) or from dark matter particles colliding and annihilating. Both theories, however, have their limitations.”

“Nonetheless, our findings strongly support the notion that the gamma-ray excess arises from dark matter annihilation.”

In their study, Dr. Libeskind and his team simulated the formation of the Milky Way galaxy under conditions akin to those in Earth’s neighboring universe.

They discovered that dark matter does not radiate outward from the galaxy’s core but is organized similarly to stars, suggesting that it could also contribute to the excess gamma rays.

“The Milky Way has long been recognized as existing within a spherical region filled with dark matter, often referred to as a dark matter halo,” explained Dr. Mourits Mikkel Mur, an astrophysicist at the Potsdam Leibniz Institute for Astrophysics and the University of Tartu.

“However, the degree to which this halo is aspheric or ellipsoidal remains unclear.”

“We analyzed simulations of the Milky Way and its dark matter halo and found that the flattening of this region sufficiently accounts for the gamma-ray excess due to self-annihilation of dark matter particles.”

“These calculations indicate that the search for dark matter particles capable of self-annihilation should be emphasized, bringing us closer to uncovering the enigmatic properties of these particles.”

A study of the survey results was published in this month’s edition of Physical Review Letters.

_____

Mikel Mur the Moor et al. 2025. Excess forms of dark matter in Fermi LAT galactic center Milky Way simulations. Physics. Pastore Rhett 135, 161005; doi: 10.1103/g9qz-h8wd

Source: www.sci.news

Everyday Sugar Could Help Uncover Dark Matter

SEI 270572247

A thin crystalline film of table sugar, or sucrose, captured using a polarized light microscope.

Carl Gough/Science Photo Library

Researchers have developed a novel method to probe dark matter utilizing expansive crystals of sucrose, or table sugar, yet their findings thus far yield nothing more than a bittersweet outcome.

Dark matter is believed to exist due to its elusive gravitational pull on galaxies; however, despite decades of exploration for potential dark matter particles, little evidence has surfaced. Historically, many searches focused on weakly interacting massive particles (WIMPs), considered leading candidates for dark matter. Yet, even the most meticulous searches have proven fruitless.

Conventional WIMP detectors aim to identify light flashes produced by interactions between dark matter particles and regular matter, assuming that these particles are relatively sizable, around 2 to 10,000 times the mass of a proton. Although this explanation is the most straightforward, the possibility exists that WIMPs are lighter, albeit creating challenges with the theory.

Recently, Federica Petricca and her team at the Max Planck Institute for Physics in Munich, Germany, have sought these lighter WIMPs utilizing a detector constructed from sugar crystals chilled to extremely low temperatures.

Very light WIMPs are expected to predominantly interact with extremely light atoms like hydrogen; however, utilizing pure hydrogen as a detector is challenging due to its low density, which diminishes interaction probabilities. On the other hand, sucrose comprises 22 hydrogen atoms in each molecule, leading to a significantly higher density than pure hydrogen.

Petricca and her colleagues initially cultivated sucrose crystals from a concentrated sugar solution over the span of a week before reducing the temperature of the crystals to 7 thousandths of a degree above absolute zero. They monitored potential dark matter interactions by employing highly sensitive thermometers to detect minimal heat increases and photon sensors to register flashes of light.

Following 19 hours of experimentation, the sugar crystals did emit light at levels comparable to interactions with larger particles; however, they did not capture the weaker signals that might indicate the presence of WIMPs.

Scientists assert that sugar crystals offer surprising sensitivity for detecting potential dark matter interactions. Carlos Blanco of Penn State notes that researchers may be able to identify subtle recoils from lightweight WIMPs. However, it remains uncertain if this experiment can effectively exclude other potential sources of crystal formation, like radioactive carbon-14, commonly present in various sugars.

CERN and Mont Blanc: Dark Matter and Frozen Matter in Switzerland and France

Get ready to be inspired by CERN, the heart of particle physics in Europe, situated near the lovely Swiss city of Geneva, where researchers manage the well-known Large Hadron Collider.

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Source: www.newscientist.com

The Heart of Our Galaxy Could Be Teeming with Dark Matter Particles

Gamma rays are detected in unusually high amounts at the center of the Milky Way galaxy

The center of our galaxy is exhibiting unusual behavior, potentially linked to dark matter. In 2009, observations from the Fermi Gamma-ray Space Telescope uncovered unexpectedly high levels of gamma ray emissions from the Milky Way’s center, a phenomenon termed galactic central gamma-ray excess (GCE). Simulations suggest these gamma rays could arise from the annihilation of dark matter particles.

The discussion surrounding the origins of GCE has intensified since its initial discovery, leading to two main theories. The first posits that it may stem from a previously unobserved population of pulsars, rapidly spinning neutron stars that emit considerable radiation.

Alternatively, it could be linked to weakly interacting massive particles (WIMPs), long considered primary candidates for dark matter. These particles seldom interact with normal matter, but a collision between two can lead to annihilation and consequently, a burst of gamma rays.

However, the dark matter explanation has lost traction recently, especially after searches for WIMPs yielded no results. “The dark matter interpretation demands greater proof due to insufficient direct evidence of its existence despite thorough investigations,” notes Jeff Grube from King’s College London.

Another factor contributing to this skepticism is that dark matter in galaxies is expected to be evenly distributed, while GCEs display a flattened distribution. Yet, new simulations by Joseph Silk and his colleagues at Johns Hopkins University in Maryland indicate that this discrepancy may not be significant.

These new simulations carefully considered the Milky Way’s history in relation to GCEs. “We know from history that our galaxy merged with smaller galaxies billions of years ago, which contributed to the formation of dark matter,” noted Silk. “No one would have anticipated that the galaxy’s center would exhibit spherical symmetry due to this history.”

The results confirmed this notion, resulting in a distorted dark matter distribution aligned with the shape of GCE, reviving the dark matter theory. However, the mystery remains unresolved, as pulsars continue to be a viable explanation. “At best, the situation is still ambiguous,” added Grube.

The current gamma-ray observatories do not possess the capability to distinguish between these two theories; however, the Cherenkov Telescope Array observatories, under construction in the Canary Islands and Chile and expected to begin operations in 2026, could provide clarity.

“In many ways, there’s a 50 percent chance that we may have discovered significant dark matter, but we require new telescopes to confirm this,” stated Silk. If GCE is indeed the result of dark matter, it could offer the best insight yet into this enigmatic substance that underpins the universe.

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Source: www.newscientist.com

Clues to Exotic Dark Matter Particles Could Be Found in LHC Data

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ATLAS Detector of the Large Hadron Collider

Xenotar/Getty Images

The theoretical particles known as axions have attracted the attention of physicists for decades, as they are significant candidates for identifying dark matter. Recent research suggests that we might not need new experiments to discover these exotic particles; evidence could already be embedded in existing data from previous particle collider experiments.

Particle colliders like the Large Hadron Collider (LHC), located at CERN near Geneva, Switzerland, discover new particles by colliding protons and ions, analyzing the resulting debris. Now, Gustabo Gilda Silveyra and his team at CERN are exploring another avenue: can we detect when a proton or ion emits a new particle during acceleration? Their findings indicate that this may indeed be possible.

The axion was theorized in the 1970s as part of a pivotal solution to a significant problem in physics. Its importance surpasses even that of antimatter. Although the ongoing search for experimental evidence of axions has not yet yielded results, it raises the possibility that other particles resembling axions might exist. Due to their incredibly low mass, they bear a close resemblance to substantial quantities of light or photons, interacting together with the LHC.

This interaction primarily occurs when protons or ions are accelerated to astonishing energy levels. As these particles approach each other, they begin to emit radiation in the form of photons, which may then collide with one another. Researchers have modeled this scenario, replacing photons with axion-like particles. Their results indicate that accelerated protons exhibit a higher likelihood of generating axion-like particles compared to accelerated ions, with both producing photons simultaneously. Consequently, the team has identified collisions between protons and lead ions as optimal for uncovering signals related to axions influencing photons. The specific proton-lead ion collisions were executed at the LHC in 2016, and the researchers propose that data from these experiments might have been previously overlooked but could contain vital hints about new axion-like particles.

Lucien Haaland Lang from University College London has remarked that this approach presents an intriguing new pathway to uncover potential undiscovered particles, though he cautions about the challenges involved. “Such collision events are rare, and we must be cautious to differentiate our findings from background processes that may inadvertently mimic the signals we seek,” he notes.

Access to older LHC data poses challenges due to updates in software, according to Da Silveira. However, he expresses optimism regarding future experiments at the LHC. “We will be able to adjust the detector to capture this specific signal,” he states.

Identifying a particle signal analogous to an axion does not equate to discovering an actual axion, thus leaving one of the major unresolved questions in physics unanswered. Nonetheless, it expands our understanding of particle physics, prompting inquiries into how new particles might interact with known counterparts and whether they might help explain the enigmatic dark matter that permeates the universe.

Journal Reference: Physical Review Letter, In print

Topics:

  • Large Hadron Collider/
  • Particle Physics

Source: www.newscientist.com

Inside the World’s Top Dark Matter Detector: What It’s Really Like to Operate

Chamkaur Ghag plays a pivotal role in the Lux-Zeplin experiment, a leading dark matter detector

Nova

Deep underground in South Dakota, the most advanced dark matter detector on Earth awaits its moment of discovery. This is the Lux-Zeplin (LZ) experiment, highlighting a vast tank of liquid xenon. Physicist Shankaur Ghag from University College London is among the key leaders in this large scientific collaboration, which aims to unravel about 85% of the universe’s mysteries that still elude us.

Currently, Ghag and his team find themselves at a crucial juncture in the quest for this elusive substance. They are considering plans for a more significant detector called xlzd, which promises to be many times the size of the LZ and even more precise. However, if neither detector can uncover the dark matter, they may need to reassess their understanding of what dark matter is. As Ghag suggests, future dark matter detectors may not be massive underground structures but rather smaller, unassuming devices. He has already devised a prototype of such a detector ahead of his upcoming talks at New Scientist Live this October.

Leah Crane: To start, why is dark matter so essential?

Chamkaur Ghag: On one side, we have all the knowledge that particles and atoms, alongside particle physics, provide about the components of matter. On the contrary, we understand gravity as well. While this may seem comprehensive, a significant issue arises when attempting to merge gravity and particle physics. Our galaxy shouldn’t exist as it does. It remains intact through gravity, which seems to derive from unseen matter. This isn’t just a tiny glue; around 85% of the universe comprises this so-called dark matter.

Why have our efforts to find it been so prolonged, with little success?

At present, we hypothesize that dark matter likely consists of what we term “wimps”—massive, weakly interacting particles that originated in the early universe. Consequently, these rarely interact with other particles, providing only a faint signature, which necessitates a large detector for detection. The larger these detectors are, the greater the chance that dark matter particles will pass through them. Additionally, they must be extremely quiet since even slight vibrations can obscure the signal.

We discuss the theoretical landscape of dark matter, which encompasses the range of masses and characteristics such particles could possess. We’ve already excluded certain regions of this landscape, making it essential to delve even deeper underground with larger detectors to explore where dark matter may still exist.

This painstaking endeavor requires minimizing background noise. For instance, many metals emit small radioactive levels, necessitating rigorous efforts to reduce construction material noise. The LZ detector boasts the lowest background noise and the highest level of radio-purity on the planet.

The LZ is currently the most sensitive detector we have. How does it function?

In essence, it operates as a double-walled thermos, containing several meters of liquid xenon. This xenon resides within a reflective tank, equipped with light sensors positioned above and below. Additionally, an electric field exists within this tank. When a wimp collides with a xenon nucleus, it generates a brief flash of light. However, due to the electric field, it causes the electrons to split apart, producing a second flash from the nucleus.

This two-signal output enables us to ascertain the exact location of an event. The intensity of both the primary and secondary flashes informs us about the microphysics of whether the interaction was caused by a wimp or an unrelated phenomenon, such as gamma rays. To ensure optimal detection, we are positioned miles underground to shield against cosmic rays and also encapsulated in an aquarium to safeguard against the surrounding rock.

This endeavor is undoubtedly complex. What has been the most challenging aspect of making it operational?

In an earlier experiment with a smaller prototype called Lux, I understood what was required to create an instrument tenfold more sensitive. Bringing that theoretical knowledge into practice proved challenging. For me, the toughest challenge lay in ensuring the instrument remained clean and quiet enough to achieve required sensitivity. When deployed with the LZ, it occupies a vast area equivalent to a football pitch, where it must tolerate only a gram of dust spread across its surface.

What is it like working with such an ultra-clean detector underground?

The environment, once a gold mine, retains its industrial atmosphere. You don a hard hat, descend a mile down, and then trek to the lab. Upon entering the lab, you lose sense of the surroundings; it transforms into a clean room filled with computers and equipment—essentially a lab devoid of windows. But the journey underground feels otherworldly.

Outer Detectors of the Lux-Zeplin Experiment

Sanford Underground Research Facility/Matthew Kapust

Historically, wimps have been the primary suspect for dark matter. At what point do we consider the wimp hypothesis invalid if we find no evidence?

Should we construct the XLZDs, the larger detectors intended for this purpose, and reach a point where they fail to detect wimps, it would be hard to sustain the idea of a standard wimp existing if we must venture beyond the capabilities of those instruments. However, until that happens, wimps are still in the game. The void between our current findings and those of the XLZD remains intriguing.

We’ve also developed a much smaller, entirely different detector for dark matter. Can you tell me more about it?

We’ve engineered 150 nanometer wide glass beads coated with lasers. This highly sensitive force detector can determine interactions in three dimensions, allowing us to ascertain which direction an event originated from. This capability is significant as it enables us to filter out terrestrial background influence, such as radioactive decay from geological materials.

This concept seems far removed from large detectors like the LZ. What’s the logic behind its creation? Will we see further advancements in smaller detectors?

Large-scale underground experiments, while large and sensitive, can paradoxically limit sensitivity due to their size. For instance, when a dark matter particle collides with my xenon detector, it may produce 10 photons. A smaller tank can capture all of them, but in a larger tank, these photons could bounce around and only a few are detected.

Furthermore, when a dark matter particle interacts with my detector, it only generates two photons initially. In this scenario, the maximal signal from a detector akin to the LZ diminishes. This has spurred the motivation to search for low-mass dark matter particles beyond the LZ’s detection range, leading us toward alternative detection methods.

If dark matter were to be discovered, what implications would that hold for physics and our understanding of the universe?

The implications would be two-fold: it would conclusively provide answers to what constitutes 85% of the universe, and it would challenge the standard model of particle physics, which currently outlines the known components of reality. Thus, if we discovered dark matter, it may offer the first glimpse beyond this conventional framework. Up until now, we’ve had no solid evidence to deviate from the standard model—this would serve as the first ray of hope.

Topics:

  • Dark Matter/
  • Particle Physics

Source: www.newscientist.com

Dark Plants as Alternatives to Street Lights? Not a Chance!

These succulent plants emit a shimmering glow after being infused with phosphor particles that absorb and gradually release light.

Liu et al., Matter

There are some product ideas that elicit just a sigh, while others I genuinely dislike. The fluorescent plants created by injecting leaves with glowing substances definitely fall into the latter category for me.

These plants are developed by researchers at the Agricultural University of South China. Recent research indicates that these plants exhibit “extraordinary brightness” and represent a move towards a “sustainable and environmentally friendly plant-based lighting solution.”

The quest to create glowing plants has spanned decades. A notable challenge is intensifying their glow for visibility. A Kickstarter project in 2013 amassed nearly $500,000 but ultimately failed to deliver on its promises.

Last year, US biotech firm Light Bio introduced the Firefly Petunia, the first genetically modified plant available for retail. They claim the plants shine “like moonlight”, but judging by social media images, it seems we’re far from a full moon effect.

The difficulty in producing glowing plants stems from plants deriving energy from light, but photosynthesis is notoriously inefficient. Estimates suggest most plants capture under 2% of the light that strikes them, and much of that energy is used for growth, leaving little to emit light.

This limitation means that energy captured from photosynthesis can never produce a plant bright enough to replace street lights. This inefficiency likely explains why most animals harness energy from plants rather than growing under the burden of photosynthesis (and also why placing solar panels on farmland promotes crop transformation into biofuels).

Consequently, several research groups have attempted to integrate sustained phosphors directly into mature plants. These compounds mimic the glow of stars in the night sky and can emit light after being charged.

Certain sustained phosphors can be significantly more efficient than photosynthesis, letting more light escape from an equal input. However, even distribution within the leaves poses challenges. Recently, Chinese researchers discovered that this kind of distribution could be more easily achieved in succulents like Echeveria “Mebina,” enabling vibrant fluorescent plants of various hues through manual injection of phosphors into each leaf.

This approach feels like a superficial gimmick. I won’t deny my interest in genuinely glowing plants. While you can find the Firefly Petunia available outside the US, I view giving plants a shine through direct injection of glowing substances as a shortcut. At the very least, this glow fades as the plants mature. There’s also a concern about possible contamination when these plants are disposed of.

While this practice may not be as unethical as dyeing aquarium fish, it’s certainly less appealing than dyeing roses. (And no, I’m not having an Alice in Wonderland moment—painted roses do exist.) Furthermore, the team’s paper does not address the environmental or safety implications of plants containing elevated levels of phosphor. I reached out to the researchers for clarification but had yet to receive a response at the time of writing.

If scientists could genetically engineer plants to produce their own biodegradable phosphors that last, this could turn into an entirely different scenario. This capability could even enhance photosynthesis efficiency. Allowing plants to temporarily “store” light would help mitigate fluctuations in light levels, converting unusable wavelengths into usable ones, thereby maintaining photosynthesis into the night. One day, entire fields might illuminate the darkness.

For now, I don’t wish to see a synthetic glowing plant derived from phosphor injections hit store shelves. I hope that never happens, yet I worry there’s a chance it might.

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Source: www.newscientist.com

Ganymede, Jupiter’s Moon, May Function as a Massive Dark Matter Detector

View of Ganymede from NASA’s Juno spacecraft

junocam/nasa/jpl-caltech/swri/msss/kalleheikki kannisto

Ganymede, one of Jupiter’s moons, has the potential to act as a significant dark matter detector, with upcoming space missions possibly unveiling unique dark matter craters on its ancient terrain.

Researchers typically seek dark matter by looking for lightweight particles that seldom interact with normal matter, employing large, insulated underground detectors. Alternatively, another category of dark matter particles could grow from the size of a basketball to that of an asteroid, but these are infrequent and interact rarely with conventional matter. To detect these hefty dark matter particles, a detector of lunar or planetary scale is necessary to account for their scarcity.

William Derocco from the University of Maryland has proposed that Ganymede, the solar system’s largest moon, may hold clues to these large dark matter particles. His research indicates that they could create a unique crater on the moon’s icy surface, preserved for millions of years due to its stable geology.

Derocco estimates the extent to which these giant dark matter particles penetrate Ganymede’s thick ice layers, finding that they reach the subterranean oceans, fostering unique minerals deeper than a standard asteroid might.

Future missions, such as NASA’s Europa Clipper and ESA’s JUICE, might be able to identify these dark material craters from orbit. Derocco believes these features will be relatively small and distinct, separated from other geological formations. He suggests that “if an underground intrusion radar is used, it may reveal this melted ice column extending down through the ice.”

Utilizing a moon-sized dark matter detector could help identify particles that elude detection on Earth, according to Zachary Picker from UCLA. He states, “Experiments on Earth struggle to find dark matter particles the size of a bowling ball. Particles the size of a refrigerator or car have interactions that are too infrequent.”

The proposal is thorough and well-reasoned, as noted by Bradley Cabana from the University of Cantabria in Spain. “There’s no compelling physical rationale to assume the existence of such massive dark matter particles,” he states. “It’s about exploring all possibilities.” He describes these as extraordinary objects, incredibly dense and held together by formidable forces from obscure sectors.

Topics:

  • Dark matter/
  • Space exploration

Source: www.newscientist.com

The Dark History of Fictional Female Robots

2JD8W56 Alicia Vikander, Ex Machina, 2014,

Alex Garland’s 2015 film Ex Machina and Sierra Greer’s Annie Bot (featured below) uphold the long tradition of female robots

Maximum Film/Alamy

This year, the Arthur C. Clarke Award for the year’s best SF fiction novel was granted to Sierra Greer’s recent work, Annie Bot. Throughout the story, Annie, a sensuous sex robot designed to revere a self-centered owner, gradually cultivates a unique personality. Yet, she is not the first artificial woman to embark on this journey. The earliest fictional female robots were simple mechanical toys, yet over time they have evolved into complex beings akin to their human counterparts.

Artificial beings have a deep-rooted history across cultures. “Every society across the globe has crafted narratives about automata for centuries,” says Lisa Yaszek, a scholar at Georgia Tech. These stories generally fit into three categories; while most depict automated laborers or weaponry, the creations of female robots typically align with domestic and sexual themes. An instance from Greek mythology, Galatea, embodies the ideal woman who comes to life when her creator, Pygmalion, falls in love with her.

Historically, these fictional automata have often mirrored real inventions. Novelties that mimic living beings began to emerge. By the 18th century, technological advancements rendered these creations increasingly lifelike and beautiful. Therefore, it’s no surprise that imaginations conjured up automata indistinguishable from reality. One of the unsettling visions of this was Eta Hoffmann’s 1817 tale Sandman, where the beautiful Olympia captivates Nathaniel despite her unsettling rigidity. Learning that Olympia is merely a moving doll ultimately drives Nathaniel to madness and demise.

In the 19th century, artificial women were often relegated to similar roles. Real women were generally expected to provide domestic services for men. In 1886, in The Night Before the Future, Auguste Villiers imagined a contemporary Pygmalion who constructs a flawless mechanical woman, annoyed by the flaws of real women. Alice W. Fuller lampooned this idea in a 1895 short story, Wife Manufactured to Order. The protagonist abandons his opinionated girlfriend in favor of the machine, yet finds himself exasperated by the robot’s mindless adoration.

By 1972, Ira Levin questioned what fate would await real women if robots could assume their roles.

This vision of an absolutely compliant Galatea has persisted through decades of fiction. “The ideal is an extremely obedient, accommodating, available woman,” outlines My Fair Woman: Female Robots, Androids, and Other Artificial Beings.

When writers envisioned automata, societal anxieties increased during the Industrial Revolution, worrying that new machines could outpace human capabilities. Fiction like Samuel Butler’s 1872 novel Erewon hinted at machines evolving their own cognitive abilities. By the dawn of the 20th century, these concerns peaked with two significant works of fiction.

Playwright Karel Čapek’s 1920 work R.U.R. depicted a world striving to elevate all people to the upper echelons of society by delegating labor to synthetic beings he called “robots.” The term robota means serf or forced labor. As foreseen by Butler’s Erewon, the robots in R.U.R. eventually rise against their creators.

Shortly thereafter, Thea von Harbou released Metropolis, adapted into Fritz Lang’s groundbreaking 1927 film. In it, female robots are designed to resemble human women of the working class. While the human Maria advocates for unity and peace, her robotic counterpart incites chaos and destruction.

Ten years later, author Leicester Del Rey introduced Helen O’Loy, presenting a mechanical femme fatale in the form of the synthetic housewife Helen, who develops feelings akin to Robot Maria. In mid-century fiction, such bots often eclipsed more rebellious counterparts. The Twilight Zone featured another robotic wife, while the Jetsons boasted the reliable Rosie the Robot maid.

Yet, the illusion of domestic happiness proved fragile. By 1972, Ira Levin posed a chilling question on what would happen if robots replaced real women. In his novel The Stepford Wives, Joanna discovers that the men in her community are murdering their outspoken wives and substituting them with docile, mechanical replicas.

In subsequent decades, franchises like Terminator and The Matrix tackled fears surrounding the technological replacement of humans—a concern that had loomed since the Industrial Revolution. However, when roles lost to machines are domestic, not all women express discontent with this outsourcing. In Iain Reid’s 2018 novel Foe, a woman confronts her human husband and ultimately claims her position with a robotic replica.

Moreover, the 2010s introduced two influential artificial women. In the 2013 film Her, a man becomes infatuated with the AI named Samantha, leading to a strained relationship with a real woman. Meanwhile, 2014’s Ex Machina features an abuser who coerces his employee Caleb to evaluate the robot AVA. As Caleb develops affection for AVA, she skillfully manipulates him to secure her escape from her creator. Though neither Samantha nor AVA are malicious, they pursue their own interests, prompting questions about the implications for those around them.

Recent narratives increasingly spotlight the journeys of artificial women themselves. In Annie Bot, Annie narrates her own evolution, prioritizing her emotional growth over that of her owner. Greer illustrates that if the bot identifies as a woman, she deserves to forge her own path. A similar approach is evident in this year’s film Fellow, which focuses on the experiences of Iris, a sex robot, as she seeks autonomy—her journey towards liberation is more nuanced than Annie’s.

But what lies ahead for these artificial women (Samantha and AVA, Annie and Iris) if they assert their independence? Their future depends on the creativity of tomorrow’s writers.

Arts and Science of Writing Science Fiction

Engage in science fiction writing this weekend, focusing on the creation of new worlds and artistic expressions.

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Source: www.newscientist.com

The Eternal Planet Sustains Itself by “Consuming” Dark Matter

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In the heart of the Milky Way, the stars appear younger than expected.

NASA, Caltech, Susan Stolovy (SSC, Caltech)

Stars in the core of our galaxy may indeed be nearly immortal, harnessing dark matter for energy.

Over two decades ago, astronomers observed oddities among the stars at the Milky Way’s center. Their emitted light suggests they are younger than their mass would indicate; this phenomenon is termed the “Youth Paradox.” Furthermore, there’s a surprising scarcity of older stars in this region, referred to as the “aging difficulty problem.”

Currently, Isabelle John from the University of Stockholm and her team employed computer simulations to propose that dark matter might hold the key to resolving both issues.

It’s established that the centers of galaxies possess high densities of dark matter. The researchers simulated the interactions of dark matter particles with stars and found that upon collision with a star’s atomic nucleus, a particle loses energy and can become trapped there. If other dark matter particles are also present at the same site, they can annihilate each other, generating bursts of energy that illuminate the stars.

Stars typically age due to a lack of fusion fuel, but dark matter could serve as an extra energy source, extending their longevity. Given the substantial amount of dark matter surrounding the galactic center, this mechanism may effectively grant stars a form of immortality, according to John.

She notes that the team’s simulations are based on broad assumptions regarding dark matter and align qualitatively with historical observations. However, further empirical data could enhance our understanding, prompting additional telescope observations to gather fresh insights on dark matter and verify if the stars at the Milky Way’s core can indeed achieve eternal life, as their nature remains poorly understood.

Mark Pinne from Ohio State University emphasizes the importance of interpreting simulations of stars situated away from the galaxy’s center. He points out that since there exists comprehensive observational data on stars near Earth, the anticipated impacts of dark matter should be cross-verified with this information.

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Source: www.newscientist.com

Understanding Dark Empathy: The Science Behind the Buzzword

Luc Kordas/Millennium Images, UK

Many of us enjoy finding new ways to categorize individuals in our lives, and recently, there’s been a noticeable surge in discussions surrounding “dark empathy.” “They appear sensitive and caring, but their true intent is manipulation.” Guardian I previously shared how TikTok influencers often label it as “the most dangerous personality type.”

This month, I’ve received requests from readers seeking clarification on the science behind these trendy terms. What defines dark empathy? And how can one identify such individuals?

This notion emerged from research investigating the so-called dark triad of personality traits: psychopathy (cold, antisocial behavior), narcissism (excessive self-focus), and Machiavellianism (manipulative tendencies). Historically, the Dark Triad was associated with a lack of empathy for others.

However, this perspective shifted with a groundbreaking 2021 study by Najah Heim, a researcher at Nottingham Trent University in England. Analyzing nearly 1,000 participants, the study confirmed that many individuals with dark triad traits lacked the capacity for empathy. However, a significant subset of around 175 participants exhibited high levels of psychopathy, narcissism, and Machiavellianism while also scoring well on standard empathy measures. They noted, for instance, that they were sensitive to others’ discomfort and claimed that people’s emotions significantly affected their own moods.

Heim and her colleagues coined the term “dark empathy” to describe this group. Further studies indicated that these individuals were generally less aggressive and more extroverted than their less empathetic counterparts, yet they displayed more hostility than the average individual. The researchers concluded that, behind a seemingly genial facade, there lies a “partially hostile core.”

This discovery prompts several questions. Psychologist Distinguish distinguishes between cognitive empathy (the visceral response to witnessing others’ emotions) and emotional empathy (the ability to understand others’ perspectives). It’s still unclear if dark empathy signifies a distinct phenomenon. Researchers also remain uncertain about how the behavior of these individuals varies depending on the context.

I am eager to find answers to these inquiries, but the current literature offers little on how to effectively interact with these individuals. For now, I will remain vigilant for classical red flags of toxic behavior, such as attempts to wield emotional manipulation through flattery or threats, and work to establish clear boundaries. While terms like “Dark Empath” may sound intriguing, their behaviors can be as distressing as those exhibited by traditional bullies in your life.

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Source: www.newscientist.com