A team of astronomers has discovered an ultramassive black hole in the foreground galaxy, with a mass estimated to be over 30 billion times that of our Sun. This massive object was detected using gravitational lensing and supercomputer simulations.
Physicists discover correspondence between dense states of gluons and enormous black holes, both characterized by self-interacting force carrier particles. The study reveals universal limits on entropy and information content in these systems.
A new study reveals that intergalactic gas can activate and feed supermassive black holes at the heart of galaxies. The researchers found a direct connection between gas outside galaxies and active supermassive black holes, with misaligned gas playing a significant role in their growth.
A rare quasar triplet formed a massive black hole with a mass of 10 billion solar masses, according to recent simulations. The triple system, composed of three galaxies with supermassive black holes at their centers, is believed to be the progenitor of ultra-massive black holes.
A study of US adults found that Black men have a 50% higher death rate within 30 days of elective surgery compared to White men and women. The researchers highlight the need for better understanding of challenges facing Black men requiring surgery in the US.
Astronomers have discovered a rapidly growing supermassive black hole in the very early Universe, which provides new clues on its formation. The galaxy, named COS-87259, contains over a billion solar masses worth of interstellar dust and is forming stars at a rate 1000 times that of our Milky Way.
Researchers have developed a new model of black hole collisions that reveals nonlinear effects in gravitational waves, allowing for more accurate modeling of the behavior. This breakthrough has significant implications for understanding black hole collisions observed by LIGO and testing Einstein's general theory of relativity.
Researchers at Johns Hopkins University have conducted simulations of two black holes colliding near the speed of light, producing a remnant black hole and gravitational waves. The study reveals nonlinear effects that cannot be studied with linearized equations, suggesting current models need to be revised.
A new model developed by researchers at Columbia University and the University of Mississippi improves the accuracy of gravitational wave analysis by including nonlinear interactions. This enhanced modeling method will help scientists better understand the structure of merging black holes and test Einstein's theory of general relativity.
A team of researchers has discovered evidence of 'cosmological coupling' between black holes and the universe's expanding energy. By studying supermassive black holes in ancient galaxies, they found that these black holes gain mass over billions of years, matching predictions for black holes that cosmologically couple with vacuum energy.
A research team from the University of Southampton discovered that supermassive black holes are fueled by gas clouds from neighboring galaxies. The study found a link between misaligned gas and active supermassive black hole activity, suggesting that galaxy interactions provide a source of fuel for these phenomena.
A team of physicists has proposed a model for a repeating partial tidal disruption event, revealing the capture of a star by a supermassive black hole and its repeated stripping of material. The study provides unprecedented insight into the existence of supermassive black holes and the orbital dynamics of stars in galaxy centers.
Astronomers using Hubble observed a star's final moments as it was gobbled up by a black hole, creating a donut-shaped torus. The event provides forensic clues to the black hole homicide, with details on the debris's behavior and the accretion rate.
Scientists using ALMA discovered a rare instance of two supermassive black holes growing simultaneously near the center of a newly coalescing galaxy. This finding suggests that binary black hole pairs may be more common than previously thought, with potential implications for future gravitational wave detections.
Astronomers have discovered two ghostly Goliath black holes just 750 light-years apart, closing in on a cataclysmic meeting. The estimated population of merging supermassive black holes may be surprisingly high, generating strong gravitational waves detectable by future telescopes.
Using supercomputers and machine learning, researchers created simulations of millions of computer-generated universes to test astrophysical predictions. The study found that supermassive black holes grow in the same way as their host galaxies, revealing a long-elusive relationship.
Researchers used 69 confirmed binaries to test two origin stories of black holes, but found that the current catalog is not enough to reveal anything fundamental about their formation. The study suggests that the universe's spin and tilt can be 'spun' in different ways depending on the model used.
Researchers believe a black hole suddenly began devouring a nearby star, releasing energy and creating the brightest ever recorded TDE. The jet's direction may be pointing towards Earth, causing Doppler boosting, and could reveal insights into how supermassive black holes grow.
Researchers suggest using ancient red giant stars' winds as a potential source of material for observing the supermassive black hole. This could provide the accretion rate needed to detect the black hole, which is currently undetectable due to its low activity.
Gravitational wave observatories LIGO and Virgo captured a signal in 2019 that differed from previous measurements. Researchers found an alternative explanation: the collision occurred on a strongly eccentric path, where one black hole was initially free to move before being captured by another's gravitational field.
Astronomers used the Young Supernova Experiment to detect an intermediate-mass black hole in a dwarf galaxy, revealing its mass and providing insight into supermassive black hole growth. The study aims to improve understanding of black hole-galaxy relationships and inform theories on supermassive black hole formation.
Astronomers have discovered the closest-known black hole to Earth, a dormant stellar-mass black hole located about 1600 light-years away in the constellation Ophiuchus. This discovery was made possible by precise observations of the motion of the black hole's companion star using the Gemini Multi-Object Spectrograph instrument.
Researchers use polarized X-ray measurements to refine models of black holes swallowing matter. The new data from Cygnus X-1 reveals a pencil-shaped plasma outflow and supports the hypothesis that processes near the black hole launch jets. This insight improves understanding of gravity's effects on space-time around black holes.
Researchers at the University of Queensland have confirmed black hole quantum properties, including superposition and wildly different masses simultaneously. The study reinforces early theories by Jacob Bekenstein, postulating that black holes can only have specific mass values within certain bands or ratios.
The Canadian Medical Association Journal (CMAJ) publishes special issues on the impact of anti-Black racism on patient health and healthcare professionals. Research by Black health scholars and practitioners sheds light on systemic inequities, including cancer care disparities and gaslighting in academic medicine.
Astronomers have discovered a rare system featuring a black hole spewing a jet at a neighboring galaxy, providing insights into radio jet feedback and its impact on star formation. The unique nature of RAD12 has allowed researchers to study the interaction between the black hole's jet and the companion galaxy.
The discovery confirms the existence of precession in a binary black hole system, where one black hole distorts space-time and causes its orbit to wobble back and forth. This effect is 10 billion times stronger than previously measured, providing insights into Einstein's theory of general relativity.
Astronomers were surprised to find that a black hole is ejecting material at half the speed of light nearly three years after shredding a nearby star. The delayed outflow challenges scientists' understanding of black hole feeding behavior, with one researcher likening it to a 'black hole burping'.
A research team proposes that magnetic reconnection around black holes energizes plasma, producing copious electron-positron pairs loaded into radio jets. This explanation aligns with M87 observations and predicts short-term X-ray emission when plasma is loaded.
Scientists discovered a mechanism to generate asymmetric temperature profiles without dynamic modulation, allowing for the imitated advection of heat. This phenomenon enables thermal trapping like that observed in black holes, with potential applications in waste heat recovery and thermal funneling.
Research published by the American Psychological Association found that racially resentful white Americans are less likely to support some gun rights if they believe Black people are exercising those rights more than white people. This bias led to a quicker match of photos of white people with gun rights phrases and photos of Black peo...
A team of researchers used sophisticated imaging algorithms to reveal a thin, bright ring of light created by photons flung around the back of a supermassive black hole. The photon ring, comprising increasingly sharp sub-rings, confirms theoretical predictions and offers new ways to explore these mysterious objects.
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.
Researchers used Stampede2 supercomputer to simulate star seeding, heating effects of primordial black holes. The study found that these two effects cancel each other out, with little impact on star formation.
A new study led by Dartmouth researchers provides the clearest understanding yet of supermassive black holes' life cycles. By analyzing X-ray telescope data and a new data analysis technique, scientists found that accretion rates vary significantly depending on how obscured an object is by gas and dust ring.
Researchers found a decline in cardiovascular mortality rates for both Black and white adults over the last 20 years. However, significant disparities in cardiovascular mortality between Black and white adults continue to exist, particularly among younger Black women and those living in highly-segregated areas.
A team of astronomers, known for debunking black hole discoveries, found a dormant stellar-mass black hole in the Large Magellanic Cloud. The newly discovered black hole is at least nine times the mass of the Sun and orbits a hot star weighing 25 times the Sun's mass.
A team of experts finds a dormant stellar-mass black hole in the Large Magellanic Cloud, a neighbor galaxy to our own. The star that formed the black hole vanished without any sign of a powerful explosion.
Researchers at UC Berkeley have detected a possible free-floating black hole in the Milky Way galaxy using gravitational microlensing. The object's mass is estimated to be between 1.6 and 4.4 times that of the sun, but its nature as a black hole or neutron star remains uncertain.
A team of physicists discovered that clouds of ultralight particles around rotating black holes leave a characteristic imprint on gravitational waves. This finding suggests the existence of new particles with very low mass, predicted by several theories beyond the Standard Model of particle physics.
Astronomers used the Cosmic Evolution Survey to discover active supermassive black holes in distant galaxies. These findings suggest that a supermassive black hole can disrupt gas and prevent star formation, leading to the sudden end of galaxy star formation.
Researchers have found a significant number of massive black holes in dwarf galaxies, contradicting previous assumptions that they are rare. The newly discovered black holes offer insights into the life story of the Milky Way's supermassive black hole and its potential mergers with other galaxies.
A team of astronomers, including those from MIT's Haystack Observatory, has captured the light around our own supermassive black hole, revealing for the first time an image of Sagitarrius A*, the black hole at the center of the Milky Way galaxy. The resulting image reveals SgrA* in a glowing, donut-shaped ring of light.
The Event Horizon Telescope captured the first image of Sagittarius A*, a hot and dense black hole surrounded by superheated gas, improving our understanding of black holes. The Frontera supercomputer supported this achievement through innovative data-driven astronomy.
The Event Horizon Telescope (EHT) has captured the first image of Sagittarius A*, a black hole at the center of the Milky Way, revealing a ring-like structure and shadow. The observation confirms Einstein's theory of general relativity and provides new insights into giant black holes.
Researchers discover innovative method to test Unruh effect in lab settings, enabling experimentation with high-intensity lasers. They also find acceleration-induced transparency, a phenomenon that could aid in unifying Einstein's general relativity with quantum mechanics.
Researchers developed a technique to study supermassive black holes smaller than M87's by measuring the brightness of their shadows over time. The 'shadow' signal can reveal the size and shape of a black hole's event horizon, shedding light on gravity's nature.
Researchers find that black holes go through a 'hard' and 'soft' state during outbursts, with the final flash possibly indicating a brief expansion of the corona. The findings help scientists understand how supermassive black holes shape galaxy formation.
Researchers used Chandra X-Ray Observatory to detect X-ray signatures of black holes in nuclear star clusters across 108 galaxies. The study found that above a certain mass and density threshold, these clusters emit x-ray signatures indicative of a black hole at twice the rate below the threshold.
Researchers found a missing link between galaxies and quasars, discovering a supermassive black hole in archived Hubble Space Telescope data. The object, GNz7q, appears to be a black hole just starting to overpower its host galaxy in the process of becoming a quasar.
Astronomers have identified a rapidly growing black hole in the early universe, GNz7q, which is considered a crucial 'missing link' between young star-forming galaxies and the first supermassive black holes. The team used Hubble data to determine that GNz7q existed just 750 million years after the big bang, with properties consistent w...
Astronomers have been searching for low-frequency gravitational waves by monitoring pulsar pulses, but now NASA's Fermi Gamma-ray Space Telescope can also be used to detect these waves. The satellite's high-energy light provides a clearer view of pulsars and offers an independent method to detect gravitational waves.
Researchers at Brookhaven Lab propose a cosmological phase transition as the key to supermassive black hole formation in the early universe. This process, facilitated by ultralight dark matter particles, enabled efficient collapse of matter into black holes.
Researchers from Purdue University and other institutions have discovered a supermassive black hole binary system, consisting of two black holes that orbit each other. The system is significant due to its close separation, which may lead to a merger releasing massive energy in gravitational waves.
Researchers propose a new mechanism for eccentric black hole mergers, suggesting that interactions between three black holes in a flat disk environment could lead to chaotic orbits. This finding challenges previous studies on the rarity of such events.
Researchers have leveraged quantum information theory techniques to amplify entanglement in the Hawking effect, a process previously difficult to test due to the faint nature of Hawking radiation. By illuminating event horizons with appropriately chosen quantum states, they can tunably stimulate entanglement production.
For the first time, scientists have measured a large difference between a black hole's rotation axis and the axis of its orbiting binary star system. This finding forces astronomers to add a new dimension to their models, offering new insights into black hole formation and physics.
Researchers from the University of Turku found that a black hole's axis of rotation is tilted more than 40 degrees relative to the orbiting stellar body. This extreme misalignment challenges current theoretical models and opens up new prospects for studying black hole formation and evolution.
Researchers have found evidence for two supermassive black holes orbiting each other every two years, with masses hundreds of millions times larger than our sun. The quasar's radio-light brightness exhibits sinusoidal variations due to the pair's motion, providing a nearly perfect light curve.
A new Rutgers study found that anti-Black and anti-LGBTQ policies in US states are associated with increased suicide risk among young Black sexual minority men. The study highlights the need for policy reform to reduce suicide risk among this population.