Articles tagged with Neutron Stars
Astronomers confirm that a stellar corpse is the source of repeated energetic flares observed after a distant star's explosive death. The team detected at least 14 irregular light pulses over a 120-day period, likely driven by processes such as rapid rotation or strong magnetic fields.
Researchers from Helmholtz-Zentrum Dresden-Rossendorf are studying near-Earth cosmic explosions to understand their potential impact on the Earth's biosphere. They found that ejected debris can reach our solar system, with some isotopes, such as iron-60 and plutonium-244, potentially coming from supernovae or other galactic events.
Researchers observed a gamma-ray burst from a kilonova, the collision of two compact neutron stars, using the James Webb Space Telescope. The data revealed the creation of the element tellurium, which had not been recognized before, and provided new insights into the formation of heavy elements in the universe.
The James Webb Space Telescope has made its first detection of a heavy element, tellurium, in a star merger. This breakthrough allows scientists to better understand the process by which rare elements are created, and may shed light on other elements near tellurium that could be present.
Researchers detected tellurium and other essential elements needed for life in the aftermath of a gamma-ray burst, revealing insights into heavy element formation. The study provides valuable information about kilonovae and neutron star mergers, paving the way for a deeper understanding of the universe.
Researchers have created a three-dimensional computer simulation of the light emitted following a neutron star merger, producing results similar to an observed kilonova. The simulation takes into account various processes and material interactions, enabling predictions for any viewing direction.
Researchers found distinct similarities between starquakes and earthquakes, but a difference with solar flares. The team analyzed nearly 7,000 bursts from three repeater FRB sources, comparing them to earthquake and solar flare data.
A team of astrophysicists at Northwestern University has successfully simulated the process of a black hole-neutron star merger, which is believed to have produced the unprecedented gamma-ray burst GRB211211A. The simulation reveals that the post-merger black hole launches jets of material from the swallowed neutron star.
Researchers propose using gravitational wave searches to detect dark matter through neutron star effects. The study forecasts constraints on heavy dark matter particles within the next decade, offering a potential tool for testing dark matter theories.
Researchers have uncovered a living star, HD 45166, that is likely to become a magnetar, marking the discovery of a new type of astronomical object - massive magnetic helium stars. The star has an incredibly strong magnetic field, 43,000 gauss, and will end its life as a compact core with a magnetic field of around 100 trillion gauss.
Researchers discovered a new type of astronomical object - a massive magnetic helium star that may evolve into a magnetar. The star has a phenomenally powerful magnetic field, about 43,000 gauss, and will eventually collapse into a neutron star with an even stronger magnetic field.
Researchers have observed significant directed flow of hypernuclei in heavy-ion collisions, offering a new direction for studying Y–N interactions. The experiment extracted slopes of directed flow of hypernuclei and light nuclei, suggesting a similar mass number scaling.
Researchers at RHIC have observed directed flow of hypernuclei, providing insight into hyperon-nucleon interactions. The findings suggest that hypernuclei follow the same mass-scaling pattern as ordinary nuclei, implying similar nucleon-nucleon and hyperon-nucleon interactions.
Scientists at IMP used a new mass spectrometry technique to precisely measure the masses of key nuclei, including arsenic-64 and selenium-66. The newly measured data led to changes in the rp-process path, indicating lower neutron star density and higher outer shell temperatures.
A Cornell astrophysicist explains how the Imaging X-ray Polarimetry Explorer (IXPE) satellite detected polarized X-rays from a magnetar, revealing 'photon metamorphosis' – a transformation of X-ray photons. The phenomenon is a natural consequence of quantum electrodynamics under strong magnetic field conditions.
Researchers detected prompt optical emission and its transition to early afterglow of a gamma-ray burst using the Ground Wide Angle Camera Array. The study provides unique data that constrains the characteristics of the progenitor, suggesting a small stellar mass.
Scientists have created the first 2D map of wind patterns around a neutron star, revealing clues to galaxy formation. The map shows the wind's vertical structure and velocity, which is about 1 million miles per hour, and offers new insights into the influence of disk winds on galaxy evolution.
Astronomers have observed an extremely rare and aspherical Fast Blue Optical Transient (FBOT) explosion 180 million light years away. The explosion, similar to a flat disc shape, challenges scientists' current understanding of stellar explosions.
The detection of GRB 221009A marks the most energetic gamma-ray burst ever observed, with a luminosity surpassing that of entire galaxies and hundreds of billions of stars. The event was followed up by space-based telescopes, including the James Webb Space Telescope, which provided insight into its properties.
Researchers have discovered a possible correlation between gravitational waves from neutron star mergers and fast radio bursts, two phenomena long shrouded in mystery. The study found that an observed FRB occurred just 2 ½ hours after a neutron star merger event, suggesting a potential link between the two events.
The discovery of Swift J1858.6-0814's neutron star confirms the presence of exotic accretionary instabilities, similar to those observed in black holes. The study reveals that these instabilities are a fundamental physical process independent of the compact object's nature.
A recent study has found that kilonovae explosions are shaped like perfect spheres, contradicting previous assumptions. The discovery may provide a new method for measuring the Universe's age, complementing existing methods and offering greater precision in distance measurements.
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.
Astronomers have uncovered a rare binary star system that has the right conditions to trigger a kilonova, an ultra-powerful explosion created by colliding neutron stars. The system, CPD-29 2176, is one of only about 10 such systems thought to exist in the Milky Way Galaxy.
A study published in Nature Astronomy suggests that a volcano-like rupture on the surface of a neutron star could have caused its sudden slowdown. The research used X-ray data from orbiting telescopes to analyze the magnetar's rotation and found evidence supporting this theory.
Researchers observed a sudden slowing of the star's angular momentum, followed by three Fast Radio Burst-like radio bursts and a month-long episode of pulsed radio emission. The synchronicity of these events suggests an association between magnetar spin-down glitches and radio emissions.
A recent astronomical observation supports theoretical modeling, revealing a new observational fingerprint of neutron-star mergers that may shed light on the production of heavy elements throughout the universe. The detection pushes our understanding of gamma-ray bursts to the limits and breaks the standard idea of these events.
A team of astrophysicists has discovered that at least some long gamma-ray bursts (GRBs) can result from neutron star mergers, contradicting the long-held belief that they solely originate from massive star collapses. This finding also sheds new light on the formation of the heaviest elements in the universe.
Two independent teams of astronomers detected the unexpected hallmarks of a kilonova after a long gamma-ray burst, challenging the prevailing theory that long GRBs exclusively come from supernovae. The discovery was made possible by the proximity of the event and the sensitivity of telescopes like Gemini North.
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.
A recent gamma-ray burst has been identified as a kilonova, shedding light on the merging of neutron stars and black holes. The event produced an excess of infrared light and lasted about a minute, contradicting the typical short duration of such explosions.
Researchers discovered a long-duration gamma-ray burst that defied prevailing theories, leading to the proposal of a new model for its origin. The unusual burst was found to have characteristics similar to those of short-duration bursts, challenging current understanding of gamma-ray burst formation.
Researchers create most extensive inventory to date of SGRB host galaxies, finding 85% come from young, actively star-forming galaxies. The study also reveals more SGRBs occurred earlier in the universe's history and were spotted far outside their host galaxies.
Physicists at Goethe University have developed over a million equations of state to model neutron star structure. These models reveal that 'light' neutron stars have a soft mantle and a stiff core, while 'heavy' stars have a stiff mantle and a soft core.
According to new research led by the University of Bath, some short-duration gamma-ray bursts are triggered by the birth of supramassive stars, not black holes. This discovery may offer a new way to locate neutron star mergers and gravitational wave emitters.
A new study published in Science found that a highly magnetised dead star, known as a magnetar, is likely to have a solid surface with no atmosphere. The research team used data from the NASA satellite IXPE to observe the polarisation of X-ray light emitted by the star, which revealed a signature consistent with a solid crust.
Researchers have developed a new model that combines nuclear physics and string theory to describe the transition to dense and hot quark matter in neutron star collisions. The model allows for the calculation of gravitational-wave signals, showing that both hot and cold quark matter can be produced.
Researchers identified rare Earth elements produced by neutron star mergers for the first time, using kilonova spectra simulations and ATERUI II supercomputer. The discovery confirms previous hypotheses about element creation and advances our knowledge of the Universe.
The European Union has awarded a €11.3 million grant to the HEAVYMETAL research project, which aims to investigate chemical element synthesis in neutron star mergers. The project brings together experts from different fields to explore kilonova explosions and decipher the details of observed spectra.
A breakthrough computer model from Chalmers University of Technology reveals the properties of an atomic nucleus, providing insights into the strong force that governs neutron star behavior. The model predicts a surprisingly thin neutron skin, which could lead to increased understanding of heavy element creation in neutron stars.
Astronomers use Hubble data combined with radio observations to measure a jet propelled by a neutron star collision, revealing it moved at an apparent velocity of seven times the speed of light.
A new study has created the first map of the Milky Way's ancient dead stars, which reveals a 'galactic underworld' stretching three times the height of the galaxy. The map shows that almost a third of objects have been flung out from the galaxy, with neutron stars and black holes formed when massive stars collapse.
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 at the University of Birmingham have developed a new model to better understand the impact of oscillations in binary neutron stars on gravitational wave detection. This could significantly improve our understanding of neutron stars and their properties.
A team led by Northwestern University captured millimeter-wavelength light from a neutron star merger for the first time, revealing one of the most energetic short-duration gamma-ray bursts. The discovery opens up new study areas, as scientists can now observe more of these events with ALMA and other telescope arrays.
Researchers recorded millimeter-wavelength light from a fiery explosion caused by the merger of a neutron star with another star, confirming it as one of the most energetic short-duration gamma-ray bursts ever observed. The results reveal that the explosion left behind one of the most luminous afterglows on record.
Astronomers have found that short gamma-ray bursts did not originate as castaways, but instead occurred in distant galaxies up to 10 billion light-years away. The discovery suggests that these events may have been more common in the past than expected and could have seeded the Universe with precious metals.
The heaviest neutron star detected has consumed nearly all the mass of its companion, growing into a record-breaking object. The study provides constraints on matter's behavior at extreme densities, potentially excluding exotic states of matter.
Devi Lal Adhikari's thesis explores mathematical connections between atomic nuclei and neutron stars, shedding light on the structure of both. His research has garnered significant attention from astrophysicists and physicists alike.
A research team from TU Darmstadt observed a neutral nucleus, the Tetra Neutron, consisting of four neutrons. The discovery provides a new system to test the nuclear force with pure neutrons, offering insights into neutron-star properties.
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.
Scientists have discovered a repeating Fast Radio Burst (FRB) with a compact source of weaker but persistent radio emission, raising new questions about the nature of these mysterious objects. The discovery challenges the usefulness of FRBs as tools for studying intergalactic space.
The NICER telescope has observed the merging of multimillion-degree X-ray spots on the surface of a magnetar, providing new insights into their behavior. The observations suggest that the crust of a neutron star can become partially molten under magnetic stress, leading to changes in pulse shape and hot spot migration.
Researchers used simulations to compare Einstein's theory and modified gravity, finding that 'dark gravity' may be equally good at explaining data from binary neutron star collisions. This could lead to the discovery of new phenomena detectable by next-generation gravitational interferometers.
A team of astronomers discovered neutron stars blowing hot, warm and cold winds while consuming matter from a nearby star. The discovery provides key information about the behaviors of these extreme cosmic objects, which contribute to the formation of new stars and galaxy evolution.
A recent analysis of the 2017 GW170817 merger suggests that a rapid spin delay may have prolonged the merger, producing excess X-ray emissions. The radiation is thought to be produced by shocked material in the circumbinary medium, hinting at a bounce from the delayed collapse.
For the first time, astronomers believe they've spotted an afterglow from a kilonova, a phenomenon resulting from the merger of two neutron stars. The discovery was made using NASA's Chandra X-ray Observatory and has sparked debate over whether it's a kilonova or black hole-related X-rays.
Basudeb Dasgupta's study shows that collective oscillations can occur only if the spectra of two neutrino flavors cross over at some energy or emission angle. This result guarantees that observation of neutrino oscillation instabilities will reveal new information from deep within the star.
Researchers have discovered a source of fast radio bursts in the vicinity of galaxy M81, adding to the ongoing mystery surrounding these enigmatic events. The findings suggest that magnetars, highly magnetized neutron stars, may be responsible for generating FRBs, but further study is needed to fully understand this phenomenon.
Researchers discovered a compact object in supernova AT2018cow, which was a product of a dying star. The team found X-ray pulses indicating an object measuring no more than 1,000 kilometers wide and with a mass smaller than 800 suns.