Physicists Suggest a Cosmic ‘Knot’ Could Have Influenced the Early Universe Briefly

Knots are prevalent in various fields of mathematics and physics today. A collaborative team of Japanese and German physicists proposes the existence of a “knot-dominated epoch” in the universe’s early days, suggesting that knots were essential building blocks during this time. This intriguing hypothesis can be investigated through gravitational wave observations. Additionally, they theorize that the conclusion of this period will involve the collapse of the knot due to quantum tunneling, leading to an Asymmetry between matter and antimatter in space.



Model proposed by Eto et al.. It suggests a brief, knot-dominated epoch when these intertwined energy fields outweighed everything else, a scenario that can be investigated through gravitational wave signals. Image credit: Muneto Nitta / Hiroshima University.

Mathematically, knots are defined as closed curves embedded in three-dimensional space and can be found not just in tying neckties but across numerous scientific disciplines today, as noted by Lord Kelvin.

Although his theory postulated that atoms are knots of etheric vortices was ultimately refuted, it sparked advancements in knot theory and its application in multiple areas of physics.

“Our study tackles one of the core mysteries of physics: why the universe is predominantly composed of matter rather than antimatter,” remarked Professor Munehito Nitta, a physicist at Hiroshima University and Keio University.

“This question is crucial as it relates directly to the existence of stars, galaxies, and ourselves.”

“The Big Bang was expected to produce equal amounts of matter and antimatter, with the intent that each particle would annihilate its counterpart, leaving only radiation.”

“Yet, the universe is overwhelmingly composed of matter, with only trace amounts of antimatter.”

“Calculations indicate that to achieve the matter we see today, only one extra particle of matter is needed for every billion matter-antimatter pairs.”

“Despite its remarkable achievements, the Standard Model of particle physics fails to resolve its inconsistencies.”

“That prediction is significantly off.”

“Unraveling the origin of the slight excess of matter, a phenomenon known as baryogenesis, remains one of the greatest unresolved enigmas in physics.”

By merging the measured baryon number minus lepton number (BL) symmetry with the Peksey-Quinn (PQ) symmetry, Professor Nitta and his associates demonstrated that the knot could have spontaneously formed in the early universe, resulting in the observed surplus.

These two well-studied extensions to the standard model address some of its most confounding gaps.

PQ symmetry offers a solution to the strong CP problem, which explains the absence of the small electric dipole moments that theories predict for neutrons, simultaneously introducing axions, a leading candidate for dark matter.

BL symmetry, conversely, elucidates why neutrinos, elusive particles that can seamlessly pass through entire planets, possess mass.

Maintaining the PQ symmetry globally, rather than merely measuring it, safeguards the delicate axion physics that addresses the strong CP problem.

In physics, “measuring” a symmetry implies allowing it to operate freely at any locale and moment in time.

However, this regional freedom requires nature to introduce new mechanisms for force transmission to clarify the equations.

By acknowledging BL symmetry, the researchers not only validated the existence of heavy right-handed neutrinos (crucial for averting anomalies in the theory and central to the primary burr formation model) but also incorporated superconducting behavior, likely providing the magnetic foundation for some of the universe’s earliest knots.

As the universe cooled following the Big Bang, its symmetry may have fractured through a series of phase transitions, leaving behind string-like defects called cosmic strings, which some cosmologists theorize may still persist.

Even though thinner than a proton, a cosmic string can stretch across a mountain.

As the universe expanded, these writhing filaments would twist and intertwine, preserving traces of the primal conditions that once existed.

The breakdown of BL symmetry formed a flux tube string, while PQ symmetry resulted in a flux-free superfluid vortex.

This contrast renders them compatible.

The BL flux tube grants the Chern-Simons coupling of the PQ superfluid vortex a point of attachment.

This coupling subsequently channels the PQ superfluid vortex into the BL flux tube, counteracting the tension that might otherwise disrupt the loop.

The outcome is a metastable, topologically locked structure known as a knot soliton.

“No prior studies had simultaneously considered these two symmetries,” notes Professor Nitta.

“In a way, our good fortune lay in this. By integrating them, we uncovered a stable knot.”

While radiation diminishes energy as waves traverse through space and time, knots exhibit properties akin to matter and dissipate energy far more gradually.

They subsequently surpassed all other forms, heralding an era of knot domination, where their energy density eclipsed that of radiation in the universe.

However, this dominance was short-lived. Ultimately, the knot succumbed to quantum tunneling, an elusive process where particles slip through energy barriers as though they were nonexistent.

This decay yielded heavy dextral neutrinos, a consequence of the inherent BL symmetry within its framework.

These colossal, elusive particles eventually transformed into lighter and more stable variations that favored matter over antimatter, shaping the universe we recognize today.

“Essentially, this decay releases a cascade of particles, including right-handed neutrinos, scalar particles, and gauge particles,” explained Dr. Masaru Hamada, a physicist at the German Electron Synchrotron Institute and Keio University.

“Among them, right-handed neutrinos are particularly noteworthy since their decay can inherently generate a discrepancy between matter and antimatter.”

“These massive neutrinos decompose into lighter particles, such as electrons and photons, sparking a secondary cascade that reheats the universe.”

“In this manner, they can be regarded as the ancestors of all matter in the universe today, including our own bodies, while knots might be considered our forebears.”

Once the researchers delved into the mathematics underlying the model—analyzing how efficiently the knot produced right-handed neutrinos, the mass of those neutrinos, and the degree of heat generated post-collapse—the observed matter-antimatter imbalance naturally emerged from their equations.

Rearranging the equations, with an estimated mass of 1012 gigaelectronvolts (GeV) for heavy dextral neutrinos, and assuming that most energy retained by the knot was utilized to generate these particles, the model yielded a natural reheating temperature of 100 GeV.

This temperature fortuitously coincides with the final opportunity for the universe to produce matter.

Should the universe cool beyond this point, the electroweak reactions that convert neutrino discrepancies into matter would cease permanently.

Reheating to 100 GeV may have also reshaped the cosmic gravitational wave spectrum, shifting it toward higher frequencies.

Forthcoming observatories such as Europe’s Laser Interferometer Space Antenna (LISA), the United States’ Cosmic Explorer, and Japan’s Decihertz Interferometer Gravitational-Wave Observatory (DECIGO) may someday detect these subtle tonal variations.

Dr. Minoru Eto, a physicist at Yamagata University, Keio University, and Hiroshima University, remarked, “The cosmic string is a variant of topological soliton, an entity defined by a quantity that remains unchanged regardless of how much it is twisted or stretched.”

“This characteristic not only guarantees stability but also indicates that our results are not confined to the specifics of the model.”

“While this work is still theoretical, we believe it represents a significant advancement towards future development, as the foundational topology remains constant.”

Although Lord Kelvin initially proposed that knots were fundamental components of matter, the researchers assert that their findings present the first realistic particle physics model in which knots could significantly contribute to the origin of matter.

“The next step involves refining our theoretical models and simulations to more accurately forecast the formation and collapse of these knots, connecting their signatures with observable signals,” said Professor Nitta.

“In particular, upcoming gravitational wave experiments like LISA, Cosmic Explorer, and DECIGO will enable the testing of whether the universe indeed experienced a knot-dominated era.”

The team’s work appears in the journal Physical Review Letters.

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Minoru Eto et al. 2025. Tying the Knot in Particle Physics. Physics. Pastor Rhett 135, 091603; doi: 10.1103/s3vd-brsn

Source: www.sci.news

Deceptive Warmth: How Volcanic Activity Influenced the Past

Geologists have identified rocks that originated in the deep sea during the early Jurassic era, around 180 million years ago, indicating a deficiency of oxygen in the ocean. These rocks were enriched with carbon atoms, specifically Carbon 12 compared to heavier carbon atoms, known as Carbon-13. Carbon-13 is denser than Carbon-12 due to having an additional neutron. Atoms belonging to the same element but with varying neutron counts are referred to as Isotopes, and the decrease in the ratio of carbon-13 to carbon-12 in rock samples is termed Negative carbon isotope distal.

Previous studies have demonstrated that during the early Jurassic, the release of photocarbon 12 into the atmosphere led to a doubling of carbon dioxide levels and an increase in ocean temperatures by 5°C, equivalent to about 9°F. This warming event is known as the Toarcian Marine Anoxia Event.

Sadly, the specific triggers for this carbon 12 release remain unclear, as there is no defined timeline for the Toarcian events. Previous estimates suggested that rock sections exhibiting low carbon isotopic ratios spanned between 300,000 to 1.5 million years. This uncertainty complicates comparisons between Toarcian warming events and more contemporary warming occurrences. Consequently, an international research team recently employed a high-precision dating technique to ascertain the exact duration of these events.

The team analyzed the Sakuradani tick section in the Tab Basin, Japan. During the early Jurassic, this region was accumulating sediment, including mud, sand, and organic matter near the coastline. The section, approximately 90 meters thick (or about 300 feet), contained layers with negative carbonate isotopic distals. Within the slope, these layers extend from around 33 meters deep to 45 meters deep.

Researchers also identified three layers of rock formed from volcanic ash both above and below the layer containing distal carbon isotopes. The upper ash layer is located about 16 meters within the rock section, while the lower ash layer can be found at approximately 49 and 51 meters. The researchers utilized volcanic ash minerals to accurately date the crystallization age of the layers. They reported that the volcanic ash layers are approximately 182.3 million, 182.5 million, and 182.9 million years old, from youngest to oldest.

These observations indicate that 62 meters (approximately 200 feet) of rock between the ash layers accumulated over a span of 400,000 years. Considering the sediment volume deposited during this time, the researchers concluded that the rock sections with distal carbon isotopes required more than 300,000 years to develop. They estimated that the duration of the Toarcian marine anoxic events was significantly shorter than earlier assumptions, lasting less than 417,000 years, with a minimum duration of 169,000 years.

With this information, the team sought to connect the Toarcian warming event and the associated carbon isotope distal to its source. They hypothesized that the event was at least partially related to volcanic activity during the early Jurassic period, which altered the composition of the surface rocks. This surge of magma to the surface could have caused the rocks to emit carbon dioxide and methane, leading to a rise in global temperatures and releasing 12 photocarbons.

The researchers concluded that volcanic activity was likely responsible for the marine anoxia events during the Toarcian period. They noted that earlier scientists had proposed volcanic mechanisms for other warming events of a similar nature. They recommend that future studies explore the direct impacts of the marine anaerobic events during the Toarcian and quantify the extent of carbon release that occurred.


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Source: sciworthy.com

Your beliefs may be influenced by your wiring, not ideology

In today’s world, partisan divisions are so sharp that it can feel like people are living in completely different realities. According to neuroscientists and political psychologists at the University of Cambridge, such as Leor Zmigrod, they are. In her new book, “The Brain of Ideology: The Radical Science of Flexible Thinking,” Dr. Zmigrod delves into new evidence suggesting that brain physiology and biology can shed light on why people are susceptible to ideology and how information is perceived and shared.

This interview has been edited for clarity and conciseness.

What is ideology?

Ideology is a narrative about how the world operates and should operate, whether in the social or natural realms. It goes beyond just being a story, providing strict guidelines on how to think, act, and engage with others. Ideology discourages deviations from its established rules.

You mention that rigid thinking is attractive. Why is that?

Ideology satisfies the desire to comprehend and explain the world. It also fulfills our need for connection, community, and a sense of belonging. Additionally, relying on established patterns and rules is a cognitively efficient strategy for navigating the world, as many ideologies insist that adhering to their rules is the morally correct way to live.

I approach this from a different angle: ideology hinders direct engagement with the world, limiting our ability to adapt to it, understand evidence, and differentiate between trustworthy and unreliable information. Ideology is seldom beneficial.

Q: The book discusses research showing that ideological thinkers can become unreliable storytellers. Can you elaborate?

This phenomenon has been observed even in children. In the 1940s, psychologist Frenkel Brunswick conducted studies on children’s bias levels and authoritarianism tendencies. When these children were given stories to recall, those with strong prejudices tended to distort the narratives to fit their biases, inventing details that aligned with their ideologies.

In contrast, children with less ideological leanings were more accurate in their story retellings, remaining faithful to the original narrative and recalling the characters’ traits correctly. This suggests that ideologically-driven individuals often incorporate fiction that reinforces their existing biases into their memories.

Do ideologues tend to integrate less information? How do they handle it differently?

Individuals inclined towards ideological thinking often resist change and nuance. This resistance is evident in tasks involving visual and verbal puzzles, where ideological thinkers struggle to adapt when the rules are altered, clinging to outdated frameworks even when they are no longer effective.

On the other hand, individuals who are more adaptable are willing to modify their behavior in response to new evidence. Ideological thinkers, however, tend to resist change and persist in applying outdated rules despite their ineffectiveness.

You have conducted a study indicating fundamental differences in brain reward circuits between ideologues and non-ideologues. Could you elaborate on your findings?

My research has revealed that individuals with strong ideological tendencies exhibit genetic traits related to dopamine distribution in the brain.

Rigid thinkers typically have lower dopamine levels in the prefrontal cortex and higher levels in the striatum. Thus, our susceptibility to rigid ideology may stem from biological variances.

Moreover, individuals with differing ideologies may exhibit variations in brain structure and function. This is particularly noticeable in brain networks associated with reward processing, emotional regulation, and error detection.

For instance, the size of the amygdala, a brain region linked to emotional processing, influences whether an individual leans towards a conservative ideology that upholds tradition and the status quo.

What are your thoughts on this?

Some researchers interpret these findings as a correlation between amygdala function and conservative ideological leanings. Both revolve around a heightened response to threats and fears.

The ambiguity surrounding these results raises the question: does our brain shape our politics, or can ideology reshape our brains?

Can we alter our wired-in ideologies?

Ultimately, individuals have the capacity to choose whether to adopt or reject ideologies.

While it may be challenging for those predisposed to rigid thinking due to genetic or biological factors, it is not predetermined or impossible to change.

Source: www.nytimes.com

Giant pandas’ plant-based diet may be influenced by MicroRNAs from Bamboo

Giant panda (Ailuropoda Melanoleuca) It belongs to the Carnivora order, but they eat mostly bamboo and their unique dietary adaptability has always been the focus of their research. Recent studies have shown that plant-derived microRNAs (miRNAs) can release nanosized vesicles (40-100 nm) released by various cell types into the extracellular space and deliver to animal organisms via exosomes that exert cross-regulatory effects on gene expression. Chinese scientists collected blood samples from three groups of pandas (boy, adult female, and adult male) to investigate the role of plant-derived miRNAs in dietary adaptation of giant pandas and extracted them from blood for small RNA analysis. Their results show that plant-derived miRNAs enter the bloodstream of giant pandas, exert cross-kingdom regulatory effects, and may play an important role in the dietary adaptation process.

Giant Panda Cube Shaoriuu and his mother Baiyun at the San Diego Zoo.

“We have shown that plant-derived miRNAs are present in the blood of giant pandas,” says Dr. Feng Li, a researcher at West Normal University of China.

“Our research has proven that bamboo, which is used as food for giant pandas, affects changes in the feeding habits of giant pandas.”

In this study, the researchers took blood samples from seven giant pandas, including three adult women, three adult men and one boy woman.

In these samples, we found 57 miRNAs that are likely to be derived from bamboo.

“Bamboo miRNAs can enter the body of giant pandas through diet, absorbed by the intestines, enter the blood circulation, and regulate the RNAs of giant pandas as they transfer information and play a role in regulating gene expression in giant pandas,” Dr. Lee said.

These plant-derived miRNAs can regulate a variety of physiological processes, including growth and development, biological rhythms, behavior, and immune responses.

“Bamboo miRNAs are also involved in regulating the smell, taste and dopamine pathways of giant pandas, and all of these are related to feeding habits,” Dr. Lee said.

“When pandas eat more bamboo as they grow, certain miRNAs accumulate, regulating gene expression and aiding in their adaptation to bamboo’s flavor.”

“These miRNAs also affect the sense of the smell of giant pandas, and may allow you to choose the freshest and most nutritious bamboo plants.”

“Therefore, bamboo miRNAs may promote the adaptation of giant pandas from carnivorous to plant-based diets.”

The authors also found that pandas of different ages and genders have different miRNA compositions in their blood.

“Only miRNAs that can play a particular role in regulating gene expression can remain in the body, and those that do not play a role are expelled,” Dr. Lee said.

“For example, some miRNAs regulate reproductive processes and can only be found in the blood of pandas of a particular gender or age.”

“The fact that miRNAs can send signals from plants to animals could open the door to researching the treatment and prevention of diseases in animals.”

“Plant miRNAs also participate in regulating the animal’s immune system, increasing the disease resistance of animals.”

Similarly, studying miRNA-induced changes in plants can also help assess and improve the safety of plant-based foods in animals and humans.

However, more research is needed to draw decisive conclusions about the potential of common miRNAs and their impact on giant pandas.

“The giant pandas are an invaluable national treasure in our country, and blood samples are not easily obtained,” concluded Dr. Lee.

“If possible, we hope to collect blood samples of young pandas who have not yet eaten bamboo for research and perhaps get more surprising results.”

result Published in the journal Veterinary Science Frontier.

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Herrington et al. 2025. Cross-Kingdom Regulation of Gene Expression in Giant Pandas via Plant-derived MiRNAs. front. Veterinarian. SCI 12; doi:10.3389/fvets.2025.1509698

Source: www.sci.news

The Permian mass extinction could have been influenced by the Mega El Niño event

Diagram of the end-Permian extinction event, where extreme temperatures may have caused forests to die off.

Richard Jones/Science Photo Library

The end-Permian extinction, 250 million years ago, may have been amplified by an El Niño event that was much stronger and longer-lasting than anything we see today.

These giant El Niño events caused extreme changes in the climate, wiping out forests and many land animals. Alexander Farnsworth At the University of Bristol, UK.

The El Niño also set off a feedback process that helped make this mass extinction so bad, he said: “There's a knock-on effect that's making these kinds of El Niños stronger and lasting longer.”

The end-Permian extinction is thought to have wiped out about 90 percent of all species living at the time, making it the worst mass extinction in history, and is widely thought to have been caused by a massive volcanic eruption in what is now Siberia.

These eruptions heated rocks rich in fossil carbon, releasing huge amounts of carbon dioxide, causing extreme global warming. Oceans became stagnant and oxygen-depleted, killing marine life.

But this doesn't explain the whole story: in particular, terrestrial species began to go extinct tens of thousands of years earlier than marine species.

A variety of ideas have been proposed to explain this, from volcanic winters to a disappearing ozone layer, but the idea that an extreme El Niño might be involved arose from studies of past ocean temperatures based on oxygen isotopes in fossils. Yadong Sun At China University of Geosciences in Wuhan.

Now, Farnsworth and his colleagues have run computer models to explore what might have happened at the end of the Permian period that could explain Sun's findings.

Currently, El Niño occurs when warm water in the western Pacific Ocean spreads eastward across the ocean surface, creating an area of ​​anomalously warm water that heats the atmosphere and affects weather across the globe.

The researchers found that before the Permian extinction began, El Niño events were probably similar in strength and duration to today, meaning abnormally warm waters were about 0.5°C (0.9°F) hotter than average and the event lasted for several months.

But these events occurred in a huge ocean called the Panthalassa, which was 30 percent larger at the equator than the present-day Pacific Ocean. This means that the area of ​​unusually warm water during El Niño was much larger than it is today, and its impact on the planet was much greater.

According to the team's model, rising carbon dioxide levels at the end of the Permian period caused El Niño events to become stronger and last longer. These events caused extreme weather changes on land and killed forests, which stopped absorbing carbon dioxide and started releasing it, leading to further warming and more extreme El Niño events.

In the ocean, the temperature changes would have been less drastic, and marine life would have had an easier time migrating to avoid them. This is why the marine extinctions occurred after more intense global warming. “The deadly extreme global warming that caused the marine extinctions was made worse by these El Niños because they stripped away carbon sinks,” says Farnsworth.

At the peak of the extinctions, El Niño temperature anomalies reached up to 4°C (7.2°F), and each event lasted for more than a decade, he says.

It's unclear whether a similar event will occur in the future — computer models vary in their predictions about how El Niño will change as the planet warms, Farnsworth said — but because El Niño occurs in a warmer world, it's already having big effects.

“The recent El Niño event has caused record temperatures and sparked a lot of wildfires,” he says, “and what worries me most is the signs of tree death in the Amazon during this El Niño event.”

Research shows that under certain climate conditions, El Niño could cause extinctions, Pedro Dinezio According to a team of researchers from the University of Colorado Boulder, such giant El Niño events don't occur today because the Pacific Ocean is smaller than the Panthalassa.

“These results are really interesting for understanding the past, rather than the near future,” Dinezio says. “To understand what El Niño will bring, we need to look at past periods when the continents were positioned similarly to the present.”

“I think this is a compelling study.” Phil Jardine Researchers at the University of Münster in Germany have discovered the first direct evidence that the ozone layer disappeared during the Permian mass extinction.

“I don't think this event and other extinction drivers, including ozone depletion, are mutually exclusive,” he says. “The scary thing about the end-Permian extinction is that a lot of things were happening at the same time, and they seemed to feed off each other in cascading ways throughout the Earth system.”

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Source: www.newscientist.com

New study finds that climate change influenced the demographics of prehistoric hunter-gatherers

Using the large number of human fossils found in Ice Age Europe, paleoanthropologists have identified a population turnover in Western Europe 28,000 years ago, isolation between western and eastern refugia between 28,000 and 14,700 years ago, and a bottleneck during the most recent Ice Age.

Artistic reconstruction of an Ice Age hunter-gatherer group. Image courtesy of Tom Björklund.

“Around 45,000 years ago, the first modern humans migrated into Europe during the Ice Age, marking the beginning of the so-called Late Paleolithic period,” said Dr Hannes Lassmann, a researcher at the University of Tübingen.

“These early populations continuously inhabited the European continent, even during the so-called Last Glacial Maximum about 25,000 years ago, a time when glaciers covered much of northern and central Europe.”

“Archaeologists have long debated how climate change and the resulting new environmental conditions affected the demographics of hunter-gatherers at the time.”

“The limited number of available fossils and the often poor molecular preservation for ancient DNA analysis have made it very difficult to draw conclusions about the influence of climatic factors on migrations, population growth, decline and extinction.”

Because teeth make up a large part of the fossil record and preserve genetic traits in their morphology, Dr. Rathman and his colleagues compiled a large dataset of 450 dentitions dating from 47,000 to 7,000 years ago.

They focused on morphological features of the teeth – small variations within the dentition, such as the number and shape of cusps on the crowns, the pattern of ridges and grooves on the chewing surfaces, and the presence or absence of wisdom teeth.

“Because these traits are heritable, they can be used to trace the genetic relationships of Ice Age humans without the need for well-preserved ancient DNA,” Dr Lassman said.

“These features are visible to the naked eye, so we also looked at hundreds of publicly available photographs of the fossils.”

The results show that between about 47,000 and 28,000 years ago, during the Middle Glacial Period, populations from Western and Eastern Europe were well connected genetically.

During the subsequent Late Glacial Period, between 28,000 and 14,700 years ago, the researchers found no genetic link between Western and Eastern Europe.

Furthermore, the analysis shows that both regions have experienced significant declines in population size and loss of genetic diversity.

“This dramatic population shift was likely caused by major climate change,” Dr Rathman said.

“Temperatures during this period fell to their lowest values ​​for the entire Upper Paleolithic, culminating in the Last Glacial Maximum, when ice sheets reached their maximum extent and covered large parts of northern and central Europe.”

“The worsening climate changed the vegetation from steppe to primarily tundra, affecting the habitat of prey animals and, consequently, the hunter-gatherers who depended on them.”

“Our findings support the long-held theory that humans were not only pushed southward by the advancing ice sheet but also isolated into isolated refugia with more favourable environmental conditions,” said Dr Judith Beier, also from the University of Tübingen.

Another notable finding of the study is the discovery that Western European populations became extinct during the transition from the Middle to Late Neoglacial and were replaced by new populations migrating from Eastern Europe.

After the Late Glacial Period, temperatures rose steadily again, the glaciers retreated, grassland and forest vegetation returned, and previously abandoned areas could be recolonized for the first time.

The team observed that during this period, the populations of Western and Eastern Europe, which had previously been isolated and significantly declining, began to grow again and migration between the regions resumed.

“Our new method makes it possible for the first time to reconstruct complex prehistoric demographic events using morphological data,” said researcher Dr Maria Teresa Vizzarri from the University of Ferrara.

“To our knowledge, this has never been accomplished before.”

“Our study provides important insights into the demographic history of Ice Age Europeans and highlights the profound impact that climatic and environmental change had on prehistoric human life,” Dr Lassmann said.

“If we want to tackle the complex environmental challenges of the future, we need to urgently learn from the past.”

of Survey results Published in the journal Scientific advances.

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Hannes Lassmann others2024. Human demography in Late Paleolithic Europe inferred from fossil dental phenotypes. Scientific advances 10(33);doi: 10.1126/sciadv.adn8129

This article has been edited based on the original release from the University of Tübingen.

Source: www.sci.news