The latest DESI data reveals a dynamic behavior of dark energy known as quintom-B, which can be explained by modified gravity theory. This study suggests that dark energy may not be a cosmological constant in the traditional sense.
The team observed an 'inside-out' growing galaxy in the early universe using the James Webb Space Telescope. This type of growth had been predicted by theoretical models but was never directly observed until now. The research found that the star formation activity is rising towards the outskirts, indicating a rapid growth rate.
Astronomers have discovered a galaxy with an unusual light signature, suggesting it may be a missing link between the universe's first stars and familiar galaxies. The galaxy's gas is outshining its stars, indicating extreme conditions that could provide insights into early galaxy evolution.
Researchers use high-resolution computer simulations and terabytes of data to detect faint signals from the Epoch of Reionization, providing insights into galaxy formation. The study sets an upper limit on when the EoR likely ended, offering a new parameter for scientists to work with as they continue to investigate the early universe.
A new study identifies regions where gravity dominates, such as the Sloan Great Wall and Shapley Supercluster, suggesting that our Milky Way likely resides in the larger Shapley basin. The research provides an unprecedented look into the gravitational landscape of the local Universe.
Astronomers have discovered a 'weird' and unprecedented galaxy in the early Universe, with its gas outshining its stars. This phenomenon could provide clues about how galaxies evolved between the Big Bang and familiar galaxies.
A new study using the Dark Energy Camera has found that early-universe quasars have surrounding companion galaxies within a distance of 15 million light-years, which is consistent with expectations. However, the team also discovered that there are no companion galaxies within 60 million light-years of the quasar.
A team of researchers using NASA's Hubble Space Telescope found more black holes than previously reported in the early universe. The new result sheds light on how supermassive black holes were created and can help scientists understand galaxy evolution.
A new study proposes that early dark energy could explain the formation of numerous bright galaxies in the early universe, resolving the 'Hubble tension' puzzle. The team modeled galaxy formation with a brief appearance of early dark energy, finding it fits observations and solves both puzzles.
Researchers unveil previously unseen properties of neutron stars through gravitational wave analysis, providing insight into internal composition and dynamic material properties. The study places observational constraints on viscosity within neutron stars.
A new study uses observations from NASA's New Horizons spacecraft to measure the cosmic optical background, a phenomenon known as the universe's glow. The results suggest that the glow is roughly 100 billion times fainter than sunlight and provides valuable insights into the history of the universe since the Big Bang.
A team of researchers observed two galaxies merging 12.8 billion years ago, forming a massive object that triggered rapid growth of supermassive black holes and starburst activity. The discovery provides new insights into galaxy/black hole formation in the early Universe.
Researchers at the Flatiron Institute and colleagues used AI-powered approach, SimBIG, to estimate five cosmological parameters with precision. The method significantly improved previous results, yielding less than half the uncertainty and closely agreeing with other estimates based on observations.
Scientists have discovered tiny, bright objects in the early universe that are packed with hundreds of millions of years old stars, defying conventional thinking about galaxy evolution. The objects also harbor surprisingly large supermassive black holes, estimated to be 100 to 1,000 times more massive than our Milky Way's black hole.
Astronomers have observed five young massive star clusters in the Cosmic Gems arc galaxy for the first time, revealing details about infant galaxies and globular cluster formation. The study uses gravitational lensing to resolve small scales in the distant galaxy, providing a unique window into the early Universe.
Researchers create a 3D printed vacuum system to trap dark matter, using ultra-cold lithium atoms to analyze the effects of domain walls. The team expects results within a year and believes this study will be an important step forward in understanding dark energy and dark matter.
The International Gemini Observatory and Subaru Telescope have discovered the most distant pair of merging quasars, seen only 900 million years after the Big Bang. The team used follow-up spectroscopy to confirm the nature of the quasar pair and their host galaxies.
Astronomers found the earliest pair of quasars, revealing a bridge of gas between merging galaxies at 900 million years after the Big Bang. This discovery clarifies the role of galaxy mergers and black hole activity in the Universe's evolution.
Researchers uncover new clues about the early universe, finding spiral galaxies were prevalent as early as 2 billion years after the universe formed. This discovery challenges previous theories and provides insight into how spiral galaxies like the Milky Way formed over time.
Researchers propose a new model that predicts far fewer primordial black holes than previously thought, which could be a strong candidate for dark matter. The study uses quantum field theory to explain the formation of these miniature black holes in the early universe.
Researchers propose a novel approach to correct the leading model of primordial black hole (PBH) formation, aligning with cosmic microwave background observations. This could imply fewer PBHs than expected, potentially affecting the dark matter theory and gravitational wave events.
Researchers witness the formation of three of the universe's earliest galaxies, 13.3-13.4 billion years ago, using the James Webb Space Telescope. The discovery contributes to understanding the universe's origins and provides insight into galaxy formation, shedding light on humanity's most basic questions.
The study uses computer simulations to test two models of the universe, finding that features observed in real galaxies can be explained by both models. However, the team also found that such features only appear in their simulations when there is both dark matter and normal matter present.
Scientists at Tohoku University and Japan Atomic Energy Agency develop experiments to manipulate the 'electron universe' geometry within magnetic materials. They successfully detected a distinct electric signal, paving the way for innovative spintronic devices.
A new study using the James Webb Space Telescope found that the universe's early galaxies developed and matured much faster than previously believed. Almost 20% of disc galaxies observed had bar formations, indicating a more settled stage in galaxy evolution.
Researchers used thermodynamics to describe the expansion of the Universe, finding that adiabatic and anisotropic effects are accompanied by cooling due to the barocaloric effect. The study proposes a novel way to investigate anisotropic effects associated with the expansion of the Universe.
Researchers from the DESI collaboration have created a largest 3D map of cosmos ever constructed, measuring expansion history with precision better than 1%. The analysis confirms basics of Lambda-CDM model but hints at possible evolution of dark energy over time.
Researchers have created the largest 3D map of the cosmos, measuring dark energy with unprecedented precision. The study provides insights into the expansion history of the young universe, with results agreeing with the Lambda CDM model but also hinting at potential differences that could indicate evolving dark energy.
The 3,200-megapixel LSST Camera will help researchers better understand dark matter and dark energy by observing the night sky in unprecedented detail. The camera's high resolution will allow it to resolve a golf ball from 15 miles away, providing valuable insights into the universe.
Astronomers have found a second-generation star in the Large Magellanic Cloud that formed in a different galaxy, offering clues about how elements were enriched in the universe. This discovery provides new hints about the early element-forming process and suggests that conditions may not be the same across all galaxies.
Astronomers have charted the largest-ever volume of the universe with a new map of active supermassive black holes, logging 1.3 million quasars in space and time. This map allows scientists to study dark matter and the universe's expansion by comparing distant quasars and their host galaxies.
A new study by University of Ottawa physicist Rajendra Gupta challenges the existence of dark matter in the universe. Using the covarying coupling constants and tired light theories, Gupta's research finds that the universe does not require dark matter to exist.
The expansion rate of the universe is faster than predicted, according to NASA's Webb and Hubble telescopes. By combining data from both telescopes, scientists have ruled out measurement errors as the cause, suggesting that new physics may be at play.
Astronomers have spotted a galaxy that stopped forming new stars over 13 billion years ago, when the universe was just 700 million years old. The 'dead' galaxy experienced a short and intense period of star formation, followed by rapid quenching.
The study reveals small galaxies produced a significant amount of ionizing photons, exceeding the threshold required for reionization. This suggests low-mass galaxies were strong candidates for sparking the process by heating and ionizing the surrounding gas.
The new CLASS maps provide further insight into linear polarization, helping scientists study the Milky Way but also studying the early universe. The results significantly improve observations, allowing for a better understanding of the cosmic microwave background and its implications on the universe's origins.
The new camera data from SPT-3G telescope promises even more detail on the universe's origins and nature. Scientists measured faint light known as cosmic microwave background, which is the afterglow of the Big Bang.
A new study found that black holes existed at the dawn of time and played a crucial role in galaxy formation. The research, using James Webb Space Telescope data, challenges classical understanding of black hole formation and suggests they may have dramatically accelerated star birth in the first 50 million years of the universe.
Researchers observed molecular gas outflow from quasar J2054-0005 using ALMA, revealing suppression of star formation in its host galaxy. The findings confirm theoretical predictions and provide strong evidence for powerful molecular gas outflows in early Universe quasars.
A team of astrophysicists used simulations to track galaxy formation near the Big Bang, including interactions between gas and dark matter. The results show that tiny, bright galaxies were formed more quickly than expected, challenging current theories about dark matter.
Researchers analyzed satellite galaxy motion around massive galaxy groups and found a notable excess of correlated pairs, suggesting recently accreted galaxies. This discrepancy with simulations implies that massive galaxy groups are younger in the real Universe.
Researchers analyzing James Webb Space Telescope images found that approximately 50-80% of early galaxies are flattened and elongated, unlike previously thought. These 'surfboard' galaxies were common in the early universe but rare nearby, suggesting they formed differently than more massive galaxies.
Researchers analyzing data from NASA's James Webb Space Telescope found that most early galaxies were flat and elongated, resembling breadsticks. These galaxies were less massive than nearby spirals and ellipticals, and are thought to be precursors to more massive galaxies like our own.
The Dark Energy Survey has released unprecedented results on the mysteries of dark energy and the expansion of the universe. The study placed the strongest constraints on the expansion rate of the universe ever obtained, consistent with the standard cosmological model but not definitive enough to rule out a more complex model.
A new study proposes that dark matter mini-halos scattered throughout the cosmos could serve as probes for primordial magnetic fields. The researchers suggest that if these fields are indeed primordial, they could cause an increase in dark matter density perturbations on small scales.
A team of researchers analyzed over one million galaxies to explore the origin of cosmic structures. They found statistically significant alignments between distant galaxy shapes and correlations between independent formation processes.
The PRIYA simulation suite provides a new model for simulating large-scale structure in the universe, constraining cosmological parameters and dark matter. The study confirms the σ8 tension between CMB measurements and weak lensing, with implications for understanding the universe's evolution billions of years after the Big Bang.
Astronomers studying two distant galaxies in the early universe reveal unprecedented molecular diversity, shedding light on the lives of prodigious star factories. By analyzing light from over 13 molecules, researchers gain insights into the physical and chemical conditions in these galaxies.
Researchers developed a machine learning technique to identify superluminous galaxies with massive black holes at their core. The algorithm predicts intense radio signals from these galaxies, which could provide insights into the physical phenomena of the early Universe.
Research reveals that the Supergalactic Plane's sparse spiral galaxies are transformed into elliptical galaxies through frequent interactions and mergers. The study used simulations to model the evolution of the Universe, finding consistency with observations of our cosmic environment.
New data from the James Webb Space Telescope reveals a surge in oxygen content within 500-700 million years after the Big Bang. This early appearance of oxygen suggests that life may have appeared sooner than previously thought.
Researchers found almost 90% of early universe galaxies had glowing gas, triggering intense star formation. The James Webb Space Telescope provided unprecedented clarity to study these infant galaxies, revealing their role in shaping the Universe.
New study finds that neglecting gravitational lensing in CMB polarization analysis leads to statistically rejected theories and biased model parameters. Researchers develop tool for correcting gravitational lensing effects, paving way for future missions to reveal nature of dark matter and dark energy.
Researchers have carried out the largest ever computer simulations to investigate the Universe's evolution, taking into account ordinary matter and dark energy. The FLAMINGO simulations provide a detailed picture of virtual galaxies and galaxy clusters, allowing for comparisons with observations from new high-powered telescopes.
Scientists will use the Simons Observatory to uncover secrets hidden in the cosmic tapestry, revealing mysteries of the universe with unparalleled precision. The observatory's completion marks a major milestone in understanding the cosmos.
Researchers propose that black holes can exist in equilibrium as 'perfect pairs' within an ever-expanding Universe. This concept challenges traditional understanding of black hole behavior and interactions.
A new method using colliding neutron stars may help resolve the discrepancy in measuring the universe's expansion rate. By analyzing the symmetry of kilonovae, astronomers can calculate distances to galaxies more accurately than current methods.
Scientists have observed 16 newly formed galaxies that exhibit significantly less heavy elements than expected, indicating a lack of time for element creation. The findings suggest that these galaxies are still in the process of being created, contradicting the long-held equilibrium model of galaxy formation.
Astronomers used James Webb Space Telescope to discover that Milky Way-like galaxies are surprisingly common and dominated throughout the universe's history. These 'disk' galaxies formed 10 billion years ago or longer and were previously thought to be fragile in early Universe.
Researchers observed the core region of the protocluster A2744z7p9OD using JWST and detected ionized oxygen-ion light from four galaxies at a distance of 13.14 billion light-years away. The team also detected cosmic dust emissions from three of the four galaxies, indicating that many first-generation stars have completed their lives.