Lifeboat Foundation

Astounding simulation shows magnetic fields create fluffy, not flat, accretion disks around supermassive black holes, altering our understanding of black hole dynamics.

A team of astrophysicists from Caltech has achieved a groundbreaking milestone by simulating the journey of primordial gas from the early universe to its incorporation into a disk of material feeding a supermassive black hole. This innovative simulation challenges theories about these disks that have persisted since the 1970s and opens new doors for understanding the growth and evolution of black holes and galaxies.

Continue reading “Caltech Astrophysicists Flip Black Hole Theories With Stunning New Simulations” »

Fermium studies indicate nuclear shell effects diminish as nuclear mass increases, emphasizing macroscopic influences in superheavy elements.

Where does the periodic table of chemical elements end and which processes lead to the existence of heavy elements? An international research team has conducted experiments at the GSI/FAIR accelerator facility and at Johannes Gutenberg University Mainz to investigate these questions.

Their research, published in the journal Nature, provides new insights into the structure of atomic nuclei of fermium (element 100) with different numbers of neutrons. Using forefront laser spectroscopy techniques, the team traced the evolution of the nuclear charge radius and found a steady increase as neutrons were added to the nuclei. This indicates that localized nuclear shell effects have a reduced influence on the nuclear charge radius in these heavy nuclei.

Microorganisms—bacteria, viruses and other tiny life forms—may drive biological variation in visible life as much, if not more, than genetic mutations, creating new lineages and even new species of animals and plants, according to Seth Bordenstein, director of Penn State’s One Health Microbiome Center, professor of biology and entomology, and the Dorothy Foehr Huck and J. Lloyd Huck Endowed Chair in Microbiome Sciences.

Bordenstein and 21 other scientists from around the world published a paper in Science, summarizing research that they said drives a deeper understanding of biological variation by uniting life’s seen and unseen realms.

Continue reading “Q&A: Holobiont biology, a new concept for exploring how microbiome shapes evolution of visible life” »

In this work, we analyzed in detail the motion of thousands of stars within each cluster,” said Alessandro Della Croce. “It quickly became clear that stars belonging to different populations have distinct kinematic properties…

How do stars form and evolve inside globular clusters? This is what a recent study published in Astronomy & Astrophysics hopes to address as an international team of researchers conducted a groundbreaking examination of star populations that reside within globular clusters, which consists of a densely packed group of stars pulled together by gravity, with the densest part in the center of the cluster. This study holds the potential to help researchers better understand the formation and evolution of stars and star populations in these unique environments throughout the cosmos.

For the study, the researchers conducted a 3D kinematic analysis of stars and star populations within 16 Galactic globular clusters (GCs) to determine the movements of stars and star populations within these clusters and how this causes the cluster to evolve over time. Since astronomers hypothesize that globular clusters are almost as old as the universe itself, they offer a unique opportunity to study some of the oldest stars in the universe, as well. In the end, the researchers found the rotation and orbital behaviors of stars were based on their light properties.

Continue reading “Unveiling the Evolution of Globular Clusters: A 3D View of Stellar Kinematics” »

What is the origin of fast radio bursts (FRBs) and what can this teach us about the galaxies where they reside? This is what a recent study published in Nature hopes to address as a team of researchers investigated how FRB signals that originate from magnetars could reside in galaxies outside the Milky Way with the goal of better understanding the processes responsible for producing FRBs, and specifically the galaxies they inhabit. Since FRBs and magnetars remain some of the most mysterious objects in the universe, this study holds the potential to help researchers gain greater insight into not only their formation and evolution, but also how this bodes for finding life beyond Earth.

“The immense power output of magnetars makes them some of the most fascinating and extreme objects in the universe,” said Kritti Sharma, who is a PhD Candidate at Caltech and lead author of the study. “Very little is known about what causes the formation of magnetars upon the death of massive stars. Our work helps to answer this question.”

For the study, the researchers used the Deep Synoptic Array (DSA-110) to analyze 30 galaxies where FRBs have been confirmed to exist with the goal of ascertaining comparing the properties of each galaxy to the FRBs they produce. While researchers have long hypothesized that FRBs are produced in galaxies of all sizes that are actively forming stars, the researchers discovered a higher number of FRBs were produced in larger galaxies as opposed to smaller galaxies. They concluded that this was likely due to larger galaxies being more metal-rich, also known as metallicity, whereas smaller galaxies tend to have smaller metallicities.

A new statistical analysis by researchers at the University of Arizona suggests that color vision evolved in animals around 500 million years ago, long before the evolution of colorful fruits and flowers, which started sprouting 200 to 350 million years ago. The researchers focused on what they term “conspicuous colors”—basically, the ones kids are likeliest to select in a 16 pack of Crayolas—red, orange, yellow, blue and purple.

Around 150 million years ago, presumably to capitalize on the well-established prevalence of color vision, species began evolving warning coloration. And 50 million years later, there was an evolutionary explosion of both warning and sexual coloration. Although the reasons behind this evolutionary burst are still unclear, the researchers identified three warning signal animal vectors behind it: ray-finned fishes, birds and lizards.

Additionally, warning coloration is much more widespread among species than sexual coloration, likely because colorful animals do not themselves need to have color vision to signal the danger they pose to other, color-sensitive species. Sexual color signals, on the other hand, are confined to vertebrate and arthropod species that have well-developed color vision.

The brain is a marvel of efficiency, honed by thousands of years of evolution so it can adapt and thrive in a rapidly changing world. Yet, despite decades of research, the mystery of how the brain achieves this has remained elusive.

Our new research, published in the journal Cell, reveals how neurons – the cells responsible for your childhood memories, thoughts and emotions – coordinate their activity.

Continue reading “The Mystery of How Neurons Control The Brain Has Finally Been Solved” »

White holes, the theoretical opposites of black holes, could expel matter instead of absorbing it. Unlike black holes, whose event horizon traps everything, white holes would prevent anything from entering. While no white holes have been observed, they remain an intriguing mathematical possibility. Some astrophysicists have speculated that gamma ray bursts could be linked to white holes, and even the Big Bang might be explained by a massive white hole. Although the second law of thermodynamics presents a challenge, studying these singularities could revolutionize our understanding of space-time and cosmic evolution.

After reading the article, Harry gained more than 724 upvotes with this comment: “It amazes me how Einstein’s theory and equations branched off into so many other theoretical phenomena. Legend legacy.”

Black holes may well be the most intriguing enigmas in the Universe. Believed to be the collapsed remnants of dead stars, these objects are renowned for one characteristic in particular – anything that goes in never comes out.

Using data from NASA’s JWST and Chandra X-ray Observatory, a team of U.S. National Science Foundation NOIRLab astronomers have discovered a supermassive black hole at the center of a galaxy just 1.5 billion years after the Big Bang that is consuming matter at a phenomenal rate — over 40 times the theoretical limit. While short lived, this black hole’s ‘feast’ could help astronomers explain how supermassive black holes grew so quickly in the early Universe.

Supermassive black holes exist at the center of most galaxies, and modern telescopes continue to observe them at surprisingly early times in the Universe’s evolution. It’s difficult to understand how these black holes were able to grow so big so rapidly. But with the discovery of a low-mass supermassive black hole feasting on material at an extreme rate, seen just 1.5 billion years after the Big Bang, astronomers now have valuable new insights into the mechanisms of rapidly growing black holes in the early Universe.

LID-568 was discovered by a cross-institutional team of astronomers led by International Gemini Observatory/NSF NOIRLab astronomer Hyewon Suh. They used the James Webb Space Telescope (JWST) to observe a sample of galaxies from the Chandra X-ray Observatory’s COSMOS legacy survey. This population of galaxies is very bright in the X-ray part of the spectrum, but are invisible in the optical and near-infrared. JWST’s unique infrared sensitivity allows it to detect these faint counterpart emissions.