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We Might Be Completely Wrong About Reality

Space. Time. Matter. What is reality? And if it’s so fundamental, why do we all experience it so differently? Join us for a marathon through the discoveries and paradoxes that suggest modern physics is pointing to a deeply uncomfortable truth: that our picture of the universe is far from complete, and what we think about reality may be completely wrong.

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00:00 Reality Is Already Broken
00:57 Scientists Build a Window into the Fourth Dimension
23:16 The Physicist Who Says Reality Is Not What It Seems
1:28:45 The Black Hole Paradox That Keeps Physicists Awake at Night
1:50:40 Sean Carroll: The Many Worlds of Quantum Mechanics
2:46:40 What are the foundations of reality?

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Fundamental constraints to the logic of living systems

Excellent review in which Solé et al. explore how physical/mathematical constraints may determine what subset of biological systems could theoretically evolve in the universe. Lots of fascinating ideas applying concepts like Turing machines, cellular automata, McCulloch-Pitts networks, energy minimization, and phase transitions to multiscale biological and evolutionary phenomena!

I found the description of how parasites almost inevitably emerge and drive increased biodiversity in computational models of evolution particularly fascinating. Interestingly, I recall this idea was featured in the Hyperion Cantos novels during an explanation of the history of artificial intelligence in their fictional universe!


Abstract. It has been argued that the historical nature of evolution makes it a highly path-dependent process. Under this view, the outcome of evolutionary dynamics could have resulted in organisms with different forms and functions. At the same time, there is ample evidence that convergence and constraints strongly limit the domain of the potential design principles that evolution can achieve. Are these limitations relevant in shaping the fabric of the possible? Here, we argue that fundamental constraints are associated with the logic of living matter. We illustrate this idea by considering the thermodynamic properties of living systems, the linear nature of molecular information, the cellular nature of the building blocks of life, multicellularity and development, the threshold nature of computations in cognitive systems and the discrete nature of the architecture of ecosystems. In all these examples, we present available evidence and suggest potential avenues towards a well-defined theoretical formulation.

Jupiter’s Galilean moons may have gained life’s building blocks at birth

Southwest Research Institute was part of an international team that demonstrated how complex organic molecules (COMs), key chemical precursors to life, could have been incorporated into Jupiter’s Galilean moons during their formation. The team’s findings have resulted in complementary studies published in The Planetary Science Journal and Monthly Notices of the Royal Astronomical Society, offering new insights into the potential for life in the Jovian system.

How complex organics can form Carbon-rich compounds containing oxygen, nitrogen and other elements are necessary for living matter to form. Laboratory experiments have shown that COMs can form when icy grains containing methanol or mixtures of carbondioxide and ammonia are exposed to either ultraviolet radiation or moderate heating under conditions found in protoplanetary disks. These disks of gas and dust surround newly formed stars that eventually form planets.

“By combining disk evolution with particle transport models, we could precisely quantify the radiation and thermal conditions the icy grains experienced,” said Dr. Olivier Mousis of SwRI’s solar system science and exploration division, who is lead author of one of the two studies. “Then we directly compared our simulations with other laboratory experiments that produce COMs under realistic astrophysical conditions. The results showed that COM formation is possible in both the protosolar nebula environment and Jupiter’s circumplanetary disk.”

Galactic islands of tranquility: ‘Little red dots’ may have brewed life’s building blocks

Astronomers have found that both the core of our Milky Way and the earliest proto-galaxies in the universe share a surprising trait: They are unusually calm and quiet in terms of harsh radiation. This tranquility is not just a cosmic curiosity; it may be essential for forming complex molecules that provide the ingredients of life.

A new study published in The Astrophysical Journal Letters highlights how the Milky Way’s center and mysterious early proto-galaxies known as “little red dots” (LRDs) harbor massive black holes within peaceful, dust-and gas-rich environments. These conditions create natural laboratories for prebiotic chemistry, suggesting that the universe may have supported life’s chemical precursors far earlier than previously imagined.

The work was led by Professor Remo Ruffini and Professor Yu Wang from the International Center for Relativistic Astrophysics Network (ICRANet) and the Italian National Institute for Astrophysics (INAF).

Space Weather Could Be Hiding Alien Signals

Dr. Vishal Gajjar: “If a signal gets broadened by its own star’s environment, it can slip below our detection thresholds, even if it’s there, potentially helping explain some of the radio silence we’ve seen in technosignature searches.”


What steps can be taken to identify why we haven’t received radio signals from an extraterrestrial intelligence, also called technosignatures? This is what a recent study published in The Astrophysical Journal hopes to address as a team of scientists investigated potential explanations regarding why humanity continues hearing silence from technosignatures. This study has the potential to help scientists and the public better understand the shortcomings and enhancements that can be made in the search for intelligent life beyond Earth.

For the study, the researchers used a series of computer models to simulate how radio signals leaving extrasolar star systems could be influenced by a myriad of factors, specifically space weather coming from the host star. This study comes as SETI and other researchers worldwide continue to come up empty regarding identifying technosignatures. The goal of the study was to ascertain potential reasons while putting constraints on both how and where to search for technosignatures.

In the end, the researchers ascertained that space weather plays a role in altering the outgoing radio signals by dispersing them, as opposed to the radio signals maintaining a fixed beam. The team ascertained that M-dwarf stars, which constitute approximately 75 percent of the stars in the Milky Way Galaxy while being smaller and cooler than our Sun, are prime targets for searching for technosignatures. This is due to their space weather, which is far more active than stars like our Sun, dispersing the radio signals.

The Simulation Argument Was Never Actually Debunked — And The Math Is Getting Worse

In 2017, headlines around the world declared the simulation hypothesis dead. Physicists had debunked it, the articles said. We could all move on. There was one problem. The paper they cited never mentioned the simulation hypothesis. The debunking was invented by journalists who never read the research. And in the years since, the actual physics has gotten significantly worse.

This documentary follows that physics all the way down.

We begin with what really happened in 2017 — the Ringel-Kovrizhin paper, what it actually proved, and Scott Aaronson’s correction that nobody shared. Then we examine Nick Bostrom’s original 2003 trilemma, the real math behind it, and why two decades of attacks from Sean Carroll, Lisa Randall, and Sabine Hossenfelder have failed to break it. Every critique concedes something. Every attempted kill shot narrows the escape routes.

From there, we trace the physics of information through three remarkable lives. Konrad Zuse, who built the first programmable computer in his parents’ living room during the bombing of Berlin, then proposed in 1967 that the universe itself is a computation — and was ignored. John Archibald Wheeler, who lost his brother in World War Two and spent the rest of his life asking whether reality is built from information, condensing it into three words that changed physics: \.

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Cosmic Megafauna — Could Giant Alien Life Forms Exist?

Space is big—but could life out there be even bigger? Join us as we ask just how enormous alien life can get—and what it might look like.

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Credits:
Cosmic Megafauna — Could Giant Alien Life Forms Exist?
Episode 727; June 26, 2025
Written, Produced & Narrated by: Isaac Arthur.
Select imagery/video supplied by Getty Images.
Music Courtesy of Epidemic Sound http://epidemicsound.com/creator.
Stellardrone, \

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Can we grow life on Mars? Experiments show potential in simulated extraterrestrial soil

Life’s capacity to survive in simulated lunar and Martian soils has been explored in two papers published in Scientific Reports. Treating simulated lunar soil with both symbiotic fungi and worm-produced compost can significantly improve the likelihood of reproduction for chickpea plants growing in the soil, indicates one study. A separate paper suggests that some microbes may be able to absorb enough water from the atmosphere to grow in simulated Martian soil at atmospheric humidity levels comparable to those on the planet.

Lunar soil—known technically as lunar regolith —does not support healthy plant growth, as it contains high concentrations of certain metals such as aluminum and zinc, does not allow water to filter through easily, and lacks the microbiome found in Earth soils. Previous research has investigated several ways to improve the fertility of lunar soil, although plants grown in these treated soils typically display various signs of stress, including stunted growth and leaf yellowing.

Jessica Atkin and colleagues grew chickpea plants (Cicer arietinum) in samples of simulated lunar soil that they treated in two ways: by adding vermicompost —produced by red wiggler earthworms (Eisenia fetida) as they decompose biowaste—at different concentrations; and by inoculating half of the soil samples at each concentration with arbuscular mycorrhizal fungi (AMF). On Earth, AMF improve the nutrient circulation properties of soil, reduce the quantity of potentially toxic metals available for absorption by plants, and produce a protein that helps bind soil together to reduce erosion. The authors then measured the quantity and weight of chickpea seeds produced, along with the plants’ heights and root mass.

Stars like our sun may maintain the same rotation pattern for life, contrary to 45 years of theoretical predictions

Researchers at Nagoya University in Japan have conducted the most detailed simulation of the interior of stars and disproved a theory scientists have believed for 45 years: that stars switch their rotation patterns as they age, with poles rotating faster than the equator in older stars. Scientists have now found that this switch may not occur. Stars maintain solar-type rotation, spinning fast at the equator and slow at the poles throughout their lifetime. The findings are published in Nature Astronomy.

Stars come in many different sizes, temperatures, and colors, ranging from red dwarfs to massive blue giants. Solar-type stars, the focus of this study, are those similar to our sun in mass and temperature. They are medium-sized, yellow stars that provide stable conditions for billions of years, long enough for planets orbiting them to potentially develop life.

Earth rotates as one solid piece, but because the sun is made of hot gas, it rotates differentially —different parts rotate at different speeds. The equator takes about 25 days to complete one rotation while the poles take about 35 days. This is known as solar-type differential rotation.

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