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Dark energy survey scientists release analysis of all six years of survey data

The Dark Energy Survey Collaboration collected information on hundreds of millions of galaxies across the universe using the U.S. Department of Energy-fabricated Dark Energy Camera, mounted on the U.S. National Science Foundation Víctor M. Blanco 4-meter Telescope at CTIO, a program of NSF NOIRLab. Their completed analysis combines all six years of data for the first time and yields constraints on the universe’s expansion history that are twice as tight as past analyses.

The Dark Energy Survey (DES) is an international, collaborative effort to map hundreds of millions of galaxies, detect thousands of supernovae, and find patterns of cosmic structure that will help reveal the nature of the mysterious dark energy that is accelerating the expansion of our universe.

From 2013 to 2019, the DES Collaboration carried out a deep, wide-area survey of the sky using the 570-megapixel DOE-fabricated Dark Energy Camera (DECam), mounted on the NSF Víctor M. Blanco 4-meter Telescope at NSF Cerro Tololo Inter-American Observatory (CTIO) in Chile. For 758 nights over six years, the DES Collaboration recorded information from 669 million galaxies that are billions of light-years from Earth, covering an eighth of the sky.

ATLAS confirms collective nature of quark soup’s radial expansion

Scientists analyzing data from heavy ion collisions at the Large Hadron Collider (LHC)—the world’s most powerful particle collider, located at CERN, the European Organization for Nuclear Research—have new evidence that a pattern of “flow” observed in particles streaming from these collisions reflects those particles’ collective behavior. The measurements reveal how the distribution of particles is driven by pressure gradients generated by the extreme conditions in these collisions, which mimic what the universe was like just after the Big Bang.

The research is described in a paper published in Physical Review Letters by the ATLAS Collaboration at the LHC. Scientists from the U.S. Department of Energy’s (DOE) Brookhaven National Laboratory and Stony Brook University played leading roles in the analysis.

The international team used data from the LHC’s ATLAS experiment to analyze how particles flow outward in radial directions when two beams of lead ions—lead atoms stripped of their electrons—collide after circulating around the 17-mile circumference of the LHC at close to the speed of light. The findings offer new insight into the nature of the hot, dense matter generated in these collisions—with temperatures more than 250,000 times hotter than the sun’s core. These extreme conditions essentially melt the protons and neutrons that make up the colliding ions, setting free their innermost building blocks, quarks and gluons, to create a quark-gluon plasma (QGP).

J. Richard Gott — Why Did Our Universe Begin?

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That the universe began seems astonishing. What brought it about? What forces were involved? How did the laws of nature generate the vast expanse of billions of galaxies of billions of stars and planets in the structures that we see today? What new physics was involved? What more must we learn?

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John Richard Gott III is a Professor of Astrophysical Sciences at Princeton University who is noted for his contributions to cosmology and general relativity.

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Do We Actually Live Inside a Black Hole? Let’s Explore the Evidence

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Hello and welcome! My name is Anton and in this video, we will talk about the claims that we live inside a black hole.
Links:
https://en.wikipedia.org/wiki/Black_hole_cosmology.
https://arxiv.org/pdf/2505.23877
https://arxiv.org/pdf/1910.10819v2

#blackhole #unvierse #astronomy.

0:00 Is universe basically a black hole?
1:10 Defining a black hole and the universe.
2:30 How would universe end up inside a black hole?
5:00 Explanations for how this may work.
6:35 Rotation and angular momentum.
8:05 What this could explain.
9:35 Counter evidence and why it’s probably not a black hole.
13:00 Rotation explanation using the cosmic web.
14:00 Conclusions.

Enjoy and please subscribe.

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Are your memories illusions? New study disentangles the Boltzmann brain paradox

In a recent paper, SFI Professor David Wolpert, SFI Fractal Faculty member Carlo Rovelli, and physicist Jordan Scharnhorst examine a longstanding, paradoxical thought experiment in statistical physics and cosmology known as the “Boltzmann brain” hypothesis—the possibility that our memories, perceptions, and observations could arise from random fluctuations in entropy rather than reflecting the universe’s actual past. The work is published in the journal Entropy.

The paradox arises from a tension at the heart of statistical physics. One of the central pillars of our understanding of the time-asymmetric second law of thermodynamics is Boltzmann’s H theorem, a fundamental concept in statistical mechanics. However, paradoxically, the H theorem is itself symmetric in time.

That time-symmetry implies that it is, formally speaking, far more likely for the structures of our memories, perceptions, and observations to arise from random fluctuations in the universe’s entropy than to represent genuine records of our actual external universe in the past. In other words, statistical physics seems to force us to conclude that our memories might be spurious—elaborate illusions produced by chance that tell us nothing about what we think they do. This is the Boltzmann brain hypothesis.

Massive black hole mystery unlocked by researchers

It’s one of astronomy’s great mysteries: how did black holes get so big, so massive, so quickly. An answer to this cosmic conundrum has now been provided by researchers at Ireland’s Maynooth University (MU) and reported today in Nature Astronomy.

“We found that the chaotic conditions that existed in the early universe triggered early, smaller black holes to grow into the super-massive black holes we see later following a feeding frenzy which devoured material all around them,” says Daxal Mehta, a Ph.D. candidate in Maynooth University’s Department of Physics, who led the research.

“We revealed, using state-of-the-art computer simulations, that the first generation of black holes—those born just a few hundred million years after the Big Bang—grew incredibly fast, into tens of thousands of times the size of our sun.”

Vast cluster of ancient galaxies could rewrite the history of star formation

Astronomers have discovered a vast, dense cluster of massive galaxies just 1 billion years after the Big Bang, each forming stars at an intense rate from collapsing clouds of dust. Reported in Astronomy & Astrophysics by an international team, led by Guilaine Lagache at Aix-Marseille University, the structure appears to challenge existing models of how rapidly stars could have formed in the early universe.

In many newly forming galaxies, immense clouds of gas and dust collapse under their own gravity, igniting rapid bursts of star formation. This process can be studied by observing extremely distant galaxies, whose light is only now reaching Earth after traveling for more than 12 billion years.

However, these observations present a challenge for astronomers. Since dust within the distant galaxy is a strong absorber of the light produced by newly forming stars, these regions are often impossible to observe directly at visible wavelengths.

First Dawn of Universe Simulation: EWOG

From Dark till First Dawn of Universe Simulation: EWOG Quantum Gravity Theory.


🚀From Dark till First Dawn of Universe Simulation: Why EWOG is promising to the Cosmic Race! 🌌 https://lnkd.in/gFBNsKtq Ever wonder how the James Webb Space Telescope (JWST) keeps finding massive, mature galaxies that “shouldn’t exist” yet? Standard cosmology (ΛCDM) is struggling to explain this without extreme fine-tuning. But Entanglement-Weighted Operator Gravity (EWOG) provides a first-principles answer. 🧩 The “Quantum Turbo” Effect In the dense early universe, high quantum entanglement between matter and geometry temporarily boosted gravity’s strength. The Core Idea: Gravity isn’t a constant; it’s an operator weighted by entanglement (Ŵ). * Curvature from Commutators: R̂ᵤᵥ = [∇̂ᵤ, ∇̂ᵥ] * The Boosted Coupling: G_eff(a, k) = G_N [1 + α₀(1 — e⁻ᵐʳ)ℱ] This “turbo boost” allowed gas to collapse into stars 150,000 years earlier than standard models predict.

First direct evidence of Migdal effect opens new path for dark matter search

In a landmark discovery that bridges nearly a century of theoretical physics, a Chinese research team has successfully captured the first direct evidence of the Migdal effect, a breakthrough with profound implications for probing dark matter—the invisible substance thought to make up roughly 85% of the universe.

The finding, published in the journal Nature, confirms a prediction made in 1939 by Soviet physicist Arkady Migdal: When an atomic nucleus suddenly gains energy—for instance, from a collision with a neutral particle (like a neutron or a dark matter candidate)—and recoils, the rapid shift in the atom’s internal electric field can eject one of its orbiting electrons.

For nearly nine decades, this “electron ejection” process remained purely theoretical. Direct evidence proved elusive because the effect occurs on an incredibly tiny scale and is easily masked by background noise from cosmic rays and natural radiation.

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