Exploring Ultra-High-Energy Neutrinos: A Potential Window into Primordial Black Hole Explosions

Physicists from the University of Massachusetts Amherst have proposed that the ultrahigh-energy neutrinos detected by the KM3NeT experiment may indicate an exploding “sub-extreme primordial black hole,” hinting at new physics beyond the Standard Model.



The KM3NeT experiment observed neutrinos with energies around 100 PeV, and IceCube detected five neutrinos exceeding 1 PeV. The explosion of a primordial black hole may account for these high-energy neutrinos. Image credit: Gemini AI.

Black holes are a well-understood phenomenon, originating when a massive star exhausts its fuel and undergoes a supernova explosion, resulting in a gravitational force strong enough to trap light. These traditional black holes are massive and relatively stable.

However, as noted by physicist Stephen Hawking in 1970, primordial black holes potentially formed not from stars, but from the universe’s primordial conditions following the Big Bang.

Theoretical in nature, primordial black holes are dense enough that light cannot escape. Surprisingly, they are expected to be significantly lighter than the black holes observed to date.

Hawking also demonstrated that when these primordial black holes heat up, they emit particles through a phenomenon known as Hawking radiation.

“The lighter the black hole, the hotter it becomes, leading to increased particle emission,” explained Dr. Andrea Tam, a physicist at the University of Massachusetts Amherst.

“As a primordial black hole evaporates, it becomes lighter and hotter, releasing even more radiation during the explosive process.”

“What our telescope detects is, in fact, Hawking radiation.”

“If we were to witness such an explosion, we would create a comprehensive catalog of all elementary particles in existence, confirming both known particles, like electrons and quarks, and those not yet observed, including hypothesized dark matter particles.”

In 2023, the KM3NeT experiment successfully detected this elusive neutrino—a result Dr. Tam and his team had anticipated.

However, a challenge arose from the IceCube experiment, which failed to record similar phenomena or approach even a fraction of KM3NeT’s findings.

If primordial black holes are prevalent and detonating often, why are we not inundated with high-energy neutrinos? What could explain this inconsistency?

Dr. Joaquín Iguazu Juan, a physicist at the University of Massachusetts Amherst, suggested, “We believe a primordial black hole with a ‘dark charge’, termed a quasi-extreme primordial black hole, could bridge this gap.”

“Dark charge mimics standard electric force but features a heavy hypothesized electron, the dark electron.”

Dr. Michael Baker, also from UMass Amherst, remarked, “Our dark charge model is complex but may provide a more accurate depiction of reality.”

“It’s remarkable that our model explains this previously unexplainable phenomenon.”

Dr. Tam added, “Dark-charged primordial black holes possess unique properties that differentiate them from simpler primordial black hole models, allowing us to resolve all conflicting experimental data.”

The research team is optimistic that their dark charge model not only elucidates neutrino observations but also addresses the enigma of dark matter.

“Observations of galaxies and the cosmic microwave background imply the existence of some form of dark matter,” explained Baker.

“If our dark charge hypothesis holds, it could suggest a considerable number of primordial black holes, aligning with other astrophysical observations and accounting for the universe’s missing dark matter,” Dr. Iguazu-Juan stated.

“The detection of high-energy neutrinos represents a significant breakthrough,” remarked Baker.

“It opens a new window into the universe, enabling us to empirically verify Hawking radiation, gather evidence of primordial black holes, and explore particles beyond the Standard Model, while inching closer to solving the dark matter mystery.”

For more details, see the findings published in Physical Review Letters.

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Michael J. Baker and colleagues. We explain the PeV neutrino flux in KM3NeT and IceCube with quasi-extreme primordial black holes. Physics. Pastor Rhett, published online December 18, 2025. doi: 10.1103/r793-p7ct

Source: www.sci.news

Physicists Reject the Existence of Sterile Neutrinos

Researchers within the MicroBooNE (Micro Booster Neutrino) collaboration have determined, with 95% probability, that a single sterile neutrino does not exist.

Utilizing data from the MicroBooNE detector, physicists announce one of the preliminary searches for sterile neutrinos with two accelerator neutrino beams. Image credit: Gemini AI.

Neutrinos are tiny subatomic particles that seldom interact with matter, allowing them to traverse the Earth without being impeded.

Current particle physics theory recognizes three types of neutrinos: electron, muon, and tau neutrinos.

These neutrinos can transform from one type to another, a phenomenon known as oscillation.

Previous experiments had revealed neutrinos that seemed to oscillate in ways not consistent with the standard model.

To clarify this anomaly, scientists suggested a fourth type: sterile neutrinos, which interact only through gravity, complicating their detection.

“The existence of three distinct flavors of neutrinos is a fundamental aspect of the Standard Model of particle physics,” explained Dr. Andrew Mastbaum, a physicist from Rutgers University and a member of the MicroBooNE leadership team.

“Because of quantum mechanical interference, neutrinos of one flavor can eventually be detected as a different flavor, a phenomenon known as neutrino oscillation.”

“Numerous unusual findings that challenge the three-flavor model have led us to postulate the existence of an additional neutrino state, referred to as a ‘sterile’ neutrino, which does not directly interact with matter.”

In the experiment conducted by MicroBooNE, physicists investigated neutrinos from two distinct beams and analyzed their oscillations.

After a decade of data gathering and scrutiny, they uncovered no evidence of sterile neutrinos, effectively rejecting one of the leading theories for the peculiarities observed in neutrino behavior.

“This result signifies a pivotal moment,” remarked Dr. Mastbaum.

“It will ignite innovative ideas in neutrino research, helping us to better comprehend the underlying phenomena.”

“While we can rule out major possibilities, this alone does not unravel the entire mystery.”

“The Standard Model does not encompass everything, such as dark matter, dark energy, and gravity, prompting scientists to seek clues that extend beyond the model,” he observed.

“By dismissing one potential explanation, we can concentrate on alternative hypotheses that may yield significant advancements in our understanding of the universe.”

The findings will also provide valuable insights for forthcoming experiments, like the Deep Underground Neutrino Experiment (DUNE).

“Through meticulous modeling and a strategic analytical approach, the MicroBooNE team has extracted an extraordinary amount of information from this detector,” stated Dr. Mastbaum.

“In next-generation projects like DUNE, we are already utilizing these techniques to explore even more fundamental questions about the essence of matter and the nature of the universe.”

of the team results published in the journal Nature.

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Collaboration with MicroBooNE. 2025. Search for photosterile neutrinos using two neutrino beams with MicroBooNE. Nature 648, 64-69; doi: 10.1038/s41586-025-09757-7

Source: www.sci.news

NOvA and T2K Experiments Reveal Unexpected Characteristics of Neutrinos

Both the NOvA (NuMI Off-Axis νe Emergence Experiment) and T2K experiments involve launching neutrinos from a particle accelerator and detecting them after they traverse extensive underground distances. The challenges are significant: out of trillions of particles, only a few leave a trace that can be detected. Advanced detectors and software are then employed to reconstruct these rare events, offering insights into how the “flavor” of neutrinos alters as they travel.

The world’s first neutrino observation inside a hydrogen bubble chamber, captured on November 13, 1970, in a 12-foot bubble chamber at a zero-gradient synchrotron. Here, an invisible neutrino collides with a proton, resulting in three particle tracks (bottom right). The neutrino changes into a muon, marked by a lengthy orbit extending up and to the left. The shorter track represents the proton, while the third track extending down and to the left is the pion formed by the collision. Image credit: Argonne National Laboratory.

Neutrinos are among the most prevalent particles in the universe.

With no charge and minimal mass, they are notoriously difficult to detect. Yet, this very elusiveness contributes to their scientific significance.

Understanding neutrinos may shed light on one of the greatest mysteries in cosmology: the reason the universe consists of matter.

Theoretically, the Big Bang should have resulted in equal parts matter and antimatter, which would have completely annihilated each other upon meeting, releasing energy in the process.

However, during the Big Bang, an imbalance occurred, producing a greater abundance of matter, which eventually led to the formation of stars, galaxies, and life as we know it.

Physicists theorize that neutrinos hold the key to this conundrum.

There are three types, or “flavors,” of neutrinos: electron, muon, and tau, which are different versions of the same fundamental particle.

They possess a unique ability to oscillate, changing from one flavor to another as they traverse space. Studying these oscillations and examining any differences between neutrinos and their antimatter counterparts could provide insights into why matter triumphed over antimatter in the nascent universe.

“Understanding these various identities could help scientists gain insight into neutrino masses and address significant questions regarding the universe’s evolution, including why matter became dominant over antimatter,” stated Dr. Zoya Valari, a physicist at Ohio State University.

“What makes neutrinos particularly intriguing is their ability to change their ‘taste.’”

“Consider this: you buy chocolate ice cream, stroll down the street, and suddenly it turns mint, only to change again with every step you take.”

To delve deeper into this shape-shifting behavior, the NOvA and T2K experiments partnered to direct neutrino particle beams over hundreds of kilometers.

NOvA projects a beam of neutrinos from a source at Fermi National Accelerator Laboratory near Chicago, traveling 500 miles to a 14,000-ton detector in Ash River, Minnesota.

On the other hand, Japan’s T2K sends a neutrino beam 295 km from the J-PARC accelerator in Tokai to the enormous Super-Kamiokande detector situated beneath Mt. Ikenoyama.

“While our objectives are aligned, the distinct experimental designs mean that synthesizing the data yields more comprehensive insights, making the whole greater than the sum of its parts,” Dr. Valari remarked.

This study builds upon earlier findings that noted minor yet significant variations in the masses of different types of neutrinos. Researchers sought deeper clues indicating that neutrinos might operate beyond the conventional laws of physics.

One such inquiry involves whether neutrinos and their antimatter counterparts exhibit different behaviors—a phenomenon referred to as charge parity violation.

“Our results indicate that additional data are needed to adequately address these fundamental questions,” Dr. Valari said.

“This underscores the importance of developing the next generation of experiments.”

Research indicates that employing two experiments with varying baselines and energies is more likely to yield answers than relying solely on a single experiment. Consequently, consolidating results from both experiments allowed scientists to explore these urgent physics questions from diverse perspectives.

“This research is extremely complex, involving hundreds of contributors in each collaborative effort,” said John Beacom, a professor at Ohio State University.

“Collaboration in science is typically competitive, but our work together here highlights the high stakes involved.”

For further details, see the new discovery published in the journal Nature.

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NOvA collaboration and T2K collaboration. 2025. Joint neutrino oscillation analysis using T2K and NOvA experiments. Nature 646, 818-824; doi: 10.1038/s41586-025-09599-3

Source: www.sci.news

Physicists at Catlin determine the maximum weight of neutrinos

Physicists of the Karlsrue Tritium Neutrino (Catlin) experiment have reported so far the most accurate measurement of the upper mass limit of neutrinos, establishing it as 0.45 electron volts (EV), less than a millionth of the electron mass.



Interior view of the main spectrometer of catrin. Image credit: M. Zacher/Katrin Collaboration.

Neutrinos are the most abundant particles in the universe and exist as three different types or flavors: Electron Neutrino, Muon Neutrino, and Tau Neutrino.

These flavors vibrate. In other words, a single neutron can be converted to each type when it moves, providing compelling evidence that neutrinos have masses that contradict the original assumptions of massless neutrinos in the standard model.

But their exact mass remains one of the great mysteries of particle physics.

in New paper In the journal Sciencethe physicists from the Catlin collaboration present the results of the first five measurement campaigns of the Catlin experiment.

“The catrin experiment determines the mass of neutrinos by analyzing the beta decay of tritium,” they explained.

“During this decay, the neutrons are converted into protons, releasing both electron and electron antioxidant, the latter being neutrino antiparticles.”

“We can infer the mass of neutrinos by analyzing the distribution of total disintegration energy between the emitted electrons and the electron antioxidants.”

For 259 days between 2019 and 2021, Catlin physicists measured approximately 36 million electrons of energy. This is a dataset of 6 times the previous run.

The findings establish the strictest laboratory base upper limit for effective electron neutrino masses and place them below 0.45 eV at a 90% confidence level.

This result shows a third improvement in the mass limit of neutrinos, and doubles the previous limit.

“For this result, we analyzed five measurement campaigns. The total data collection from 2019 to 2021 is about a quarter of the total data expected from Catlin,” said Dr. Catlin Valerius, one of the two co-spokemens for the Catlin experiment and a physicist at the Karl-Thru Institute.

“In each campaign, we gained new insights and further optimized the experimental conditions,” said Dr. Suzanne Mertens, a physicist at the Max Planck Institute for Nuclear Physics and the Institute of Technology Munich.

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Max Aker et al. (Catlin collaboration). 2025. Direct neutrino mass measurements based on 259 days of catrin data. Science 388 (6743): 180-185; doi: 10.1126/science.adq9592

Source: www.sci.news

The Shrinkage of Neutrinos is Beneficial for Physics

On Thursday, researchers released the most accurate measurements of neutrinos, reducing the maximum possible mass of ghostly speckles of matter permeating our universe.

result, Published Science journals do not define the exact mass of neutrinos, but do not define just the upper limit. However, this discovery helps physicists get closer to understanding what is wrong with the so-called standard model. One way physicists know that it is not accurate at all is that they suggest that neutrinos have no mass at all.

In Grander Scales, learning more about neutrinos can help cosmologists fill in hazy pictures of the universe. This includes how galaxies gather and what will affect the expansion of the universe since the Big Bang.

“The new research is a great opportunity to learn more about the world,” said John Wilkerson, Chapel Hill, a physicist at the University of North Carolina and author of the new study. “And that’s what neutrinos may play a key role.”

Physicists know a few things about neutrinos. They are prolific across the universe and are actually created whenever atomic nuclei snap together or fall apart. However, they are notoriously difficult to detect because they do not carry charges.

There are three types of neutrinos, which physicists describe as flavors. And, strangely enough, they change from one flavor to another when they travel to space and time, a discovery recognized by the Nobel Prize in Physics in 2015. The underlying mechanism that allowed these transformations meant that neutrinos had to have some mass.

But that’s the case. Neutrinos are dauntingly light, and physicists don’t know why.

Revealing the exact values of neutrino masses, Alexei Lokhov, a scientist at the Karlsruhe Institute of Technology in Germany, said that new physics could lead to “some kind of portal.” “At the moment, this is the biggest limitation in the world,” he said of the team’s measurements.

Dr. Rokhov and his colleagues conducted an experiment using Karlsrue tritium neutrinos or catrine to narrow down the neutrino mass. One end of the 230-foot-long device is a heavy version of hydrogen, a source of tritium and with two neutrons in its nucleus. Tritium is unstable and collapses into helium. A neutron is converted into a proton, and in the process the electrons are ejected. It also spits out antinutrinos, the antimatter twins of neutrinos. The two require the same mass.

The original tritium mass is divided into helium, electrons, and antioxidant spoilage products. Neutrinos and anti-anti-utrinos cannot be directly detected, but the sensor on the other side of the experiment recorded 36 million electrons over 259 days and was washed away by attenuated tritium. By measuring the energy of electron movement, they were able to indirectly infer the maximum possible mass for antinutorino.

They found that the value was less than 0.45 electron volts, one million times lighter than electrons, in the unit of mass used by particle physicists.

The upper limit of mass was measured only for one flavour of neutrinos. But Dr. Wilkerson said that nailing one chunk would allow you to calculate the rest.

Latest measurements reduce the potential mass of neutrinos Previous limit Set in 2022 by Katrin Collaboration under 0.8 Electronvolts. It’s also almost twice as accurate.

University of Washington physicist Elise Nowitzky praised the Catlin team for their careful efforts, although not involved in the job.

“It’s really the power of tours,” she said of her experiments and discoveries. “I’m totally confident in their outcome.”

The Catlin team is working on further boundaries of neutrino masses from 1,000 days of data and is expected to be collected by the end of the year. This allows physicists to measure even more electrons, leading to more accurate measurements.

Other experiments also contribute to a better understanding of neutrino mass. Project 8 Seattle and deep underground neutrino experiments spread across two physical facilities in the Midwest.

Astronomers studying the structure of the universe, thought to be influenced by the vast collection of universes, have a vast collection of neutrinos that are flooded into the universe, and have their own measurements of the maximum mass of particles. However, according to Dr. Wilkerson, the boundaries that astronomers stare at the void do not match what particle physicists calculate in their lab when scrutinizing the subatomic world.

“There’s something really funny going on,” he said. “And the possible solution to that would be physics beyond the standard model.”

Source: www.nytimes.com

KM3NET continues to observe the highest energy cosmic neutrinos

The newly detected neutrino, called KM3-230213A, has an incredible energy of 220 peta-electronic (PEV), making it one of the most powerful basic particles ever detected. Its energy was about 100 million times more energy than visible photons, and about 30 times the highest neutrino energy previously detected.



Visual impressions of ultra-high energy neutrino events observed in KM3NET/ARCA. Image credit: km3net.

Cosmic neutrinos are generated near or along cosmic ray propagation pathways, leading to the generation of secondary unstable particles, which then collapse into neutrinos.

Cosmic rays interacting in the Earth's atmosphere generate atmospheric neutrinos that form the experimental background of cosmic neutrinos.

Monitor a huge amount of neutrino observatory to detect space neutrinos. Cherenkov Light It is induced by the passage of charged particles due to neutrino interactions within or near the detector.

“This high-energy neutrino is extremely rare and makes it a monumental discovery,” says Professor Miroslav Filipovich of Western Sydney University.

“This finding represents the most energetic neutrinos ever observed, providing evidence that such high energy neutrinos are being produced in the universe.”

“Detecting such extraordinary particles brings us closer to understanding the most powerful forces that shape our universe.”

Detection of KM3-230213a is KM3NET Telescopephotoelectron-filled tubes are used to capture light from charged particles generated when neutrinos interact with the detector.

“KM3NET's research infrastructure consists of two detector arrays of optical sensors deep in the Mediterranean,” the physicist said.

“The ARCA detector is located approximately 3,450 m deep off the coast of Portopalo Di Capo Passero in Sicily, Sicily, Italy, and is connected to the INFN coastal station, Nazionali Del Sud using electro-optic cables.”

“ARCA's geometry is optimized for research into high-energy cosmic neutrinos.”

“The ORCA detector is located at a depth of approximately 2,450 m in France's offshore Toulon and is optimized for studying neutrino oscillations.”

“Both detectors are under construction, but they are already working.”

The KM3-230213A event recorded light of over 28,000 photons, providing clear trajectories and compelling evidence suggesting the cosmic origin of the particles.

“KM3NET can reconstruct neutrino trajectories and energy,” says Dr. Luke Burns of Western Sydney University.

“To create neutrinos like these, like explosive stars and super-large black holes, requires extreme cosmic conditions.”

“The work of following up on the radiotelescope, like the Australia Square Kilometer Array Pathfinder, helps unlock their secrets.”

The researchers concluded that it is difficult to clearly determine its origin based on a single neutrino.

Future observations will focus on constructing clearer images of such events in order to construct clearer images of such events.

“The energy of the KM3-230213A event is much greater than the energy of neutrinos detected so far,” the scientists said.

“This suggests that neutrinos may be derived from a different cosmic accelerator than low-energy neutrinos, or this could be the first detection of cosmicogenic neutrinos. Universe.”

Team's paper Published in the February 12th issue of the journal Nature.

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KM3NET collaboration. 2025. Observation of ultra-high energy cosmic neutrinos using KM3NET. Nature 638, 376-382; doi:10.1038/s41586-024-08543-1

Source: www.sci.news

Neutrinos shatter records as they tear through the Mediterranean Ocean

Part of the undersea KM3NET neutrino detector

km3net

The incredibly powerful neutrinos that tore through a new Mediterranean particle detector have amazed physicists, offering a first glimpse into some of the universe’s most intense events, such as the collision of ultrafine black holes.

Neutrinos, sometimes known as “ghost particles,” interact minimally with matter due to their small mass and lack of charge. By placing detectors in dense mediums like water or ice, researchers hope to detect the subtle signals of neutrinos interacting with atoms and producing showers of particles. This, in turn, helps in understanding their properties.

Damian Dornick from the Centre for Particle Physics in Marseille, France, along with his team, discovered the most energetic neutrino ever recorded. Using the Cubic Kilometer Neutrino Telescope (km3net) at the bottom of the Mediterranean Sea, they detected this extraordinary neutrino on February 13, 2023. The discovery left the researchers astonished.

“Initially, we were puzzled,” he says. “As we delved deeper, we realized that this event was truly exceptional, and our excitement grew.”

The signal observed appeared as a bright, almost horizontal line on the detector, believed to be created by muons – small electron-like particles produced by neutrinos interacting with km3net’s detectors.

https://www.youtube.com/watch?v=gpuargix2u4

When the researchers tentatively published their results in 2024, they were still in the process of calculating the exact energy of the particles. “The high energy levels surprised us, as our neutrino simulations had not yet reached such levels,” says Morgan Wasco from Oxford University.

To validate their findings, researchers meticulously considered the impact of other sources of illumination on the detector, such as neutrinos generated by cosmic rays – charged particles from space. These signals are believed to surpass higher-energy neutrinos originating from more distant cosmic sources by 1 to 100 million times.

The energy of the detected neutrino was calculated to be 120 peta electron volts (PEV), about 10 times higher than the previous record set by the IceCube neutrino observatory in Antarctica. Such high-energy neutrino detections offer unique insights into the events producing them, like black hole mergers and supernova explosions.

“While cosmic rays get deflected and lose their original direction as they pass through interstellar space, neutrinos travel straight,” explains Wascko. The relatively large spatial spread of the neutrino’s trail in this case makes pinpointing the exact source challenging, but future enhancements to the telescope could potentially identify similarly powerful neutrinos and their sources.

topic:

Source: www.newscientist.com

China and the US race to study neutrinos, the mysterious ‘ghost particles’ of the cosmos

Trillions of neutrinos pass through our bodies every second. The sun produces them through nuclear fusion. The same goes for nuclear power plants. Some come from supernova explosions in space. Neutrinos are paired with antineutrinos, which scientists believe mirror the behavior of neutrinos.

As such, JUNO is designed to capture antineutrinos, specifically the antineutrinos emitted by two nuclear power plants located approximately 53 miles from the observatory.

The 13-story JUNO sphere will be filled with a special liquid called a scintillator and submerged in a cylinder of purified water, said project leader Wang Yifang, director of the China Institute of High Energy Physics.

When the antineutrinos pass through the liquid, they trigger a chemical process that produces a brief burst of light that can be picked up by sensors inside the sphere.

“This event will cause a flash that will last only about 5 nanoseconds, and we hope to capture it with thousands of photomultiplier tubes surrounding the sphere,” he says, as a worker behind him says, Mr. Wang, wearing a helmet, spoke while installing the doubler. “We hope to catch 60 events per day.”

Thanks to its approach, JUNO should be able to measure differences in antineutrino masses about 10 times more accurately than previous instruments.

First of three new neutrino observatories

JUNO is part of China’s ambitious efforts to become a global scientific powerhouse. In a speech this year, President Xi Jinping laid out plans to transform the country into a science and technology superpower by 2035.

October 11th, workers at the bottom of JUNO.Eric Baclinao/NBC News

JUNO is expected to be the first of three next-generation neutrino observatories to open over the next decade, making it a kind of spearhead in a new era of physics. In Japan, the Hyper-Kamiokande Observatory is scheduled to open in 2027. And a U.S.-backed program called the Deep Neutrino Experiment (DUNE) calls for particle accelerators to send beams of neutrinos underground from Illinois to North Dakota starting in 2027. 2031.

The three upcoming observatories are both complementary and competitors, as they all plan to use different techniques to detect particles. Each project involves extensive international collaboration aimed at advancing the field, creating new spin-off technologies and training a new wave of scientists.

“When you start these experiments, it’s not unlikely that you’ll observe something unexpected,” said Chris Marshall, an assistant professor of physics at the University of Rochester who works on the DUNE project. “Trying to unravel these very complex effects will require multiple experiments measuring things in different ways.”

The ability of each observatory to answer important physics questions depends in part on how well researchers can collaborate between and among projects. But there is growing concern among some scientists around the world that rising geopolitical tensions between the United States and China, and the resulting deterioration in their scientific relations, could hinder progress. are.

In recent years, the United States has pursued policies to prevent Chinese scientists from bringing American-based technology to the country and to prevent China from poaching its scientific stars.

Wang said the U.S. is denying visa applications for 2022 and 2023 without explanation and limiting U.S. involvement in JUNO.

“In science, cooperation and competition are good, but it can’t be all about competition,” he said.

On October 11, Mr. Wang pointed out to journalists the underlying characteristics of JUNO’s domain.Eric Baclinao/NBC News

U.S.-based scientists also said they have found new obstacles to cooperation with Chinese scientists.

“From the U.S. side, it’s becoming increasingly difficult to obtain funding for collaborations with Chinese colleagues,” Patrick Huber, director of the Center for Neutrino Physics at Virginia Tech, said in an email. It has also become much more difficult for our Chinese colleagues to obtain U.S. visas.” .

“It’s not impossible to collaborate with Chinese scientists, but it’s becoming increasingly difficult,” said Ignacio Taboada, a physics professor at the Georgia Institute of Technology who directs an existing neutrino observatory in Antarctica. “I’m working on it,” he said.

Solving the mystery of neutrinos

The data generated by JUNO could go a long way toward solving important mysteries about how and why neutrinos change shape more than other elementary particles.

Neutrinos can oscillate, or transform, between three so-called “flavors” during their travels: muon, tau, and electron. For example, the sun sends electron neutrinos toward Earth, but they can also arrive as muon neutrinos. When neutrinos interact (which rarely happens), they settle on a particular flavor.

Additionally, scientists believe that neutrinos travel as one of three different mass states, and that state helps determine the likelihood of a neutrino interacting as a particular flavor. However, it is not yet clear which state has the largest population.

Scientists also found that neutrinos and antineutrinos may deform differently as they travel, and that those differences may account for some of the imbalance in the physics between matter and antimatter in the universe. I think there is.

Journalists take photos at the top of JUNO’s sphere on October 11th.Eric Baclinao/NBC News

If so, learning more about the masses and oscillations of neutrinos and antineutrinos will help researchers find a missing page in the Standard Model of physics (the rulebook of particles and their interactions), or something that has never been known before. This could help researchers understand whether missing particles or forces are having invisible effects. role.

“Our beautiful theory of reality, the Standard Model, is not the final theory,” said Sergio Bertolucci, an Italian particle physicist and DUNE co-spokesperson. “It turns out that we need to know more about neutrinos to answer things that the standard model can’t answer.”

Wang hopes JUNO will win the race to determine the neutrino mass hierarchy before the United States and other countries.

“We just want to be good scientists. In science, being first is most important. There’s nothing to be second,” he said. “As a scientist, I can’t always be a follower. I want to have my own thing.”

Entrance to the Jiangmen Underground Neutrino Observatory in China.Eric Baclinao/NBC News

If JUNO explains the neutrino mass story before DUNE comes online, the U.S.-led project will be able to measure that question differently and confirm JUNO’s results.

DUNE’s plan is to measure neutrinos as they leave the Illinois facility, then travel 800 miles around Earth, where they can interact and oscillate. If the neutrinos arrive in South Dakota and can be detected, scientists could compare the flavor combinations of the neutrinos at the beginning and end of their journey. However, the project experienced delays and cost overruns.

“JUNO’s uniquely rich dataset, alone or in combination with other experiments, will play a key role in determining bulk orders by 2030,” said Professor Pedro Ochoa said in physics and astronomy from the University of California, Irvine.

However, several scientists involved in neutrino observation projects acknowledged that it is impossible to predict how much benefit the research will actually bring to Earth. They suggested that in the future, new technologies could be spun off, driving innovation in data-intensive computing and advancing particle accelerator science.

“We can’t make electric light by improving candles, so we need to take a step forward. We need a break,” said John C., a particle physicist at the U.S. Department of Energy’s Brookhaven National Laboratory and co-spokesperson for the DUNE project. Mary Bishai says. “Basic research inherently creates discontinuities.”

Wang put it another way, saying his work is driven by pure curiosity: “I work in ‘useless’ science.”

Source: www.nbcnews.com