The James Webb Space Telescope has refined measurements of the Hubble constant using Cepheid variables. The observations provide new insights into the universe's expansion rate and its implications for the cosmos.
University of Michigan researchers found that large cosmic structures grow at a rate slower than expected, with dark energy accelerating the universe's expansion having an opposite effect on structure growth. This discovery challenges the standard model and addresses the S8 tension in cosmology.
Researchers using ALMA detected a fully formed magnetic field in a distant galaxy, similar to nearby galaxies, which provides new insights into the formation of galactic-scale magnetic fields. The discovery suggests that intense star formation in the early Universe could have played a role in accelerating the development of these fields.
A team of researchers used the Subaru Telescope to discover 162 quasars in the early universe, including 22 that lived less than 800 million years old. The observation provides insights into the origin of supermassive black holes and their relationship with galaxies.
Astronomers have improved the accuracy of the Universe's expansion parameters, reducing uncertainty by up to 35%. This new information will help determine whether the Universe will continue expanding forever or eventually collapse in on itself.
Scientists have long debated the source of magnetic fields in the universe. New research by Columbia University researchers suggests that turbulent plasma can spontaneously generate these fields, which then amplify and spread across vast distances.
A new study by uOttawa researchers proposes a revised cosmological model that stretches galaxy formation time, making the universe 26.7 billion years old. This finding addresses the 'impossible early galaxy problem' and provides a more feasible explanation for the advanced level of development observed in ancient galaxies.
The James Webb Space Telescope has discovered the most distant active supermassive black hole to date in galaxy CEERS 1019, which existed 570 million years after the big bang. This smaller black hole is less massive than previously detected behemoths and provides insight into the early universe's formation.
Researchers used quasar data to analyze time dilation in the early universe, confirming that it was running at five times slower. By observing nearly 200 quasars, scientists were able to standardize their 'ticking' and chart the expansion of space.
A new study detects starlight from two massive galaxies hosting actively growing black holes, seen less than a billion years after the Big Bang. The findings suggest that the relationship between black holes and their host galaxies was already in place 860 million years ago.
Researchers from UNIGE have developed a new method to test the validity of Einstein and Euler's theories on the accelerating Universe expansion and dark matter. The study uses time distortion as a never-before-used measure, allowing for differentiation between the two equations.
Researchers at the University of Toronto have made a breakthrough in understanding dark matter and its impact on the universe's large-scale structure. By analyzing cosmic microwave background data and galaxy clustering patterns, they suggest that ultra-light axion particles could account for the observed lack of clumpiness.
The latest DESI data release provides a precise 3D map of the universe with high certainty. The data also sheds new light on cosmic acceleration and the nature of gravity at large scales.
New data from NASA's James Webb Space Telescope shows that galaxies' stars emitted enough light to heat and ionize the gas around them, clearing our collective view over hundreds of millions of years. The research team identified galaxies near quasars and found that they are generally surrounded by transparent regions about 2 million l...
Researchers using NASA's James Webb Space Telescope confirm the existence of JD1, a tiny galaxy typical of those that burned through hydrogen left over from the Big Bang, enabling ultraviolet light to travel through space. The discovery sheds new light on the early universe's formation and reionization process.
University of Florida astronomers discovered parity symmetry violation, a broken symmetry that explains why there's more matter than antimatter. This finding confirms the Big Bang theory and addresses the question of why something exists instead of nothing.
A team of researchers from the University of Minnesota has successfully measured the expansion rate of the Universe using data from a magnified supernova. Their findings provide new insight into the problem and bring scientists closer to obtaining the most accurate measurement of the Universe's age.
Kavli Institute researchers found that oscillon decay can generate detectable gravitational waves, offering a novel test of early Universe dynamics. This discovery provides a new window into the earliest moments of the Universe and may help address pressing cosmological questions.
Researchers from the Atacama Cosmology Telescope collaboration have created a groundbreaking new image that reveals the most detailed map of dark matter distributed across a quarter of the entire sky. The study confirms Einstein's theory of how massive structures grow and bend light, supporting the standard model of cosmology.
Indiana University researchers and collaborators have completed a six-year experiment to study the fundamental properties of neutrinos. They observed nearly 10^26 atoms over six years, pushing the boundaries of detection for this rare phenomenon.
Astronomers using NASA's Hubble Space Telescope discovered a pair of gravitationally bound quasars inside two merging galaxies when the universe was just 3 billion years old. The finding provides insights into early galaxy mergers and supermassive black holes.
Researchers have discovered a large reservoir of hot gas in the Spiderweb galaxy cluster, which is believed to be on its way to becoming a massive galaxy cluster. The detection was made using ALMA and provides valuable information about the early Universe's structure formation.
An international team of researchers has successfully demonstrated the formation of fullerene and its derivatives in the universe. The reaction involves a corannulene radical and vinyl acetylene, which deposit layers of carbon onto each other to form the desired molecules.
A team of researchers used machine learning to analyze elemental abundances in over 450 extremely metal-poor stars. The study found that 68% of these stars have a chemical fingerprint consistent with enrichment by multiple supernovae, providing the first quantitative constraint on the multiplicity of the first stars. This challenges th...
A team of researchers found the earliest evidence of heated gas in a galaxy protocluster, indicating temperatures characteristic of the present-day 'Warm-Hot Intergalactic Medium'. This discovery provides insight into the mechanisms that caused the intergalactic gas to boil up and offers a unique window into the early universe.
A series of simulations have enabled researchers to probe the heterogeneous structure of the universe by treating galaxy distribution as a collection of points. The study reveals that on large scales, the universe approaches hyperuniformity, while on smaller scales it becomes almost antihyperuniform and strongly inhomogeneous.
A University of Queensland-led research team is using an unusual caesium atom to search for dark matter particles. The team's work may also improve atomic theory calculations and technology, such as navigation systems.
A team of scientists has discovered six massive galaxies in the early universe, challenging current theories on galaxy formation. These galaxies are estimated to be as mature as the Milky Way and were found when the universe was only 3% of its current age.
Researchers found that kilonovae, caused by neutron star collisions, produce spherical explosions with symmetrical shapes. The discovery may provide a new key to fundamental physics and measuring the Universe's age.
Researchers Martin S. Sloth and Florian Niedermann introduce New Early Dark Energy (NEDE) as a solution to the Hubble tension problem, suggesting a phase transition in dark energy that explains different measurement results for the universe's expansion rate.
A team of researchers has created a highly accurate map of the universe's matter distribution, combining data from two major telescope surveys. The analysis reveals that matter is less 'clumpy' than expected, suggesting potential inconsistencies with the current standard model of the universe.
The Hydrogen Epoch of Reionization Array (HERA) team has doubled the sensitivity of its radio telescope array, providing clues to the composition of stars and galaxies in the early universe. The data suggest that early galaxies contained few elements besides hydrogen and helium.
Researchers utilized the James Webb Space Telescope to observe dense interstellar clouds, revealing a treasure trove of pristine ices from the early universe. The study provides new insights into chemical processes in one of the coldest places in the universe, offering clues on molecular origins and sulfur storage.
Researchers have measured the size-luminosity relation of galaxies less than a billion years after the Big Bang for the first time. The team used multiband imaging data from the GLASS-JWST program to study galaxy properties in rest-frame optical and UV bands.
A team of astronomers discovered 87 galaxies that could be the earliest known galaxies in the universe using data from NASA's James Webb Space Telescope. This finding suggests a revision to our understanding of galaxy formation, indicating that more galaxies may have formed earlier than previously thought.
Researchers used new data from the European Space Agency's GAIA space observatory to project the orbits of satellite galaxies into the past and future, revealing the plane form and dissolve in a few hundred million years. The findings remove one of the main objections to the validity of the standard model of cosmology.
Researchers at RIT have made a groundbreaking discovery confirming the light emitted by stars outside our galaxy is two to three times brighter than previously thought. This finding suggests a possible absence of optical light sources in the universe, potentially changing our understanding of how it formed over time.
The James Webb Space Telescope has captured infrared images of a population of red spiral galaxies at unprecedented resolution, revealing their morphology in detail. These galaxies are among the farthest known spiral galaxies and suggest that such spiral galaxies existed in large numbers in the early universe.
The event challenged scientists' understanding of gamma-ray bursts (GRBs), which are the most powerful events in the universe. The burst's high-energy light and kilonova visible and infrared light were detected by NASA's Swift Observatory and Fermi Gamma-ray Space Telescope, providing new insights into how heavy elements are created.
Astronomers have uncovered a nearby galaxy, HIPASS J1131–31, nicknamed 'Peekaboo,' which has characteristics reminiscent of galaxies in the distant, early universe. The tiny galaxy is only 20 million light-years from Earth and exhibits extreme metal-poor properties.
An international team of researchers has successfully characterized the earliest galaxies in the Universe, which formed only 200 million years after the Big Bang. The study found that these early galaxies were relatively small and dim, processing less than 5% of their gas into stars.
Researchers used India's SARAS3 radio telescope data to place limits on the mass and energy output of the first stars and galaxies, determining what they were like and weren't. The study enabled them to rule out scenarios of inefficient heaters and efficient producers of radio emissions.
Researchers have measured the size of a star dating back 2 billion years after the Big Bang, gaining insight into the stars and galaxies of the early Universe. The study used detailed images of a red supergiant supernova to reconstruct its cooling process, shedding light on how massive stars formed in galaxies during this period.
Astrophysicists have identified a potential test to rule out cosmic inflation, a theory explaining the universe's origins. The cosmic graviton background (CGB) could provide evidence against inflation if detected, and its impact on the early Universe's expansion rate could be measured by next-generation probes.
A team of astronomers used the James Webb Telescope to identify five ancient globular clusters, potentially containing the first and oldest stars in the universe. The clusters were formed close to the Big Bang, offering insights into star formation and galaxy evolution.
Achenbach, a renowned experimental physicist, will lead Jefferson Lab's Experimental Hall B, utilizing the world's most powerful accelerator to advance nuclear physics research. He aims to upgrade CEBAF and explore new experiments, including positron beams, to expand knowledge on matter and the universe.
Researchers using JWST's First Deep Field image identified the most distant globular clusters, potentially relics of the first and oldest stars. These discoveries provide a detailed look at the earliest phase of star formation, confirming JWST's power in uncovering the universe's origins.
Astronomers detect massive light burst from 'infant' Universe, revealing properties of cosmic explosions. The GRB was triggered by a space explosion that occurred when the Universe was less than 900 million years old.
Researchers have discovered young stars spiraling into the center of a massive cluster in the Small Magellanic Cloud, a satellite galaxy of the Milky Way. The spiral motion is thought to be feeding star formation in a river-like motion of gas and stars, an efficient way to fuel star birth.
Researchers propose using precision data from upcoming experiments to test the cosmological collider effect and unravel the mystery of matter's origin. They suggest that leptogenesis, a well-known mechanism, could be used to explain the imbalance between matter and antimatter in the early universe.
Astronomers propose a new method to measure the universe's expansion rate by analyzing the changes in signal properties of black hole collisions. By using the entire population of black holes as a calibration tool, scientists can directly identify and correct for errors, providing a more accurate measurement.
A new study by University at Buffalo physicists Will Kinney and Nina Stein reveals that the latest cyclic model introduces a new problem: the universe must have a beginning. This finding contradicts previous theories, which aimed to address entropy concerns by proposing endless cycles of expansion and contraction.
Researchers analyzed archive data from powerful cosmic explosions to find a new way to measure distances in the universe. They identified a class of 179 gamma-ray bursts with common features, which can be used as a cosmological tool.
A team of astronomers has developed a novel way to observe the first stars and galaxies, detecting light through the fog of the early Universe. The Square Kilometre Array will likely make images of the earliest light, but current telescopes struggle to detect the cosmological signal through hydrogen clouds.
Scientists at Kyoto University propose a novel approach using holograms to approximate the universe's expansion in de Sitter space. The model uses conformal field theory and a positive integer for the cosmological constant, enabling the identification of the first example of two-dimensional CFT.
A new Caltech project, COMAP, will peer beneath the 'tip of the iceberg' of galaxies to unveil a hidden era of star formation. The project aims to answer questions about what caused the universe's rapid increase in star production.
A team of researchers created simulations that directly recreate the full life cycle of massive galaxy protoclusters 11 billion years ago. They were able to identify five new structures and disfavor one, providing insights into the standard model of cosmology.
Researchers discovered a previously unnoticed mathematical property that could allow for a faster expansion rate while preserving other predictions. This finding suggests the existence of a 'mirror world' with similar but invisible particles interacting only through gravity.
A unique new instrument and powerful telescope allow researchers to peer into galactic nurseries at the heart of the young universe. The team used gravitationally lensed galaxies to observe two DLA clouds, determining their size and mass for the first time.
A University of Helsinki research team used holographic duality to model early universe phase transitions and their potential impact on gravitational wave signals. The study, published in Physical Review Letters, suggests that such collisions could create powerful ripples in spacetime detectable by satellite missions like LISA.