Articles tagged with Gravitational Waves
The team used the Swope telescope to discover the light produced by the merger and obtained the earliest spectra of the collision. These observations may allow scientists to explain how many of the universe's heavy elements were created.
The first-ever detection of light from a gravitational wave source has been made, shedding new light on the behavior of matter under extreme conditions. The event, caused by two neutron stars colliding and merging together, was observed using numerous telescopes around the world.
For the first time, astronomers have observed a cataclysmic cosmic event that generated gravitational waves detected on Earth. The event was the merger of two neutron stars in a galaxy 130 million light-years away, resulting in a supernova-like explosion.
Scientists directly observed two neutron stars for the first time, detecting gravitational waves and a burst of gamma rays. The event allowed researchers to calculate the expansion rate of the universe and verify Einstein's prediction that gravitational waves travel at the speed of light.
The detection of light from a neutron star merger reveals the formation of heavy elements like gold and platinum. The observations support theoretical predictions and provide new insights into astrophysics.
For the first time, scientists have detected the collision of two neutron stars using both gravitational waves and light. The historic discovery ushers in a new era in astronomy with multi-messenger astronomy, confirming theoretical predictions and providing new mysteries to understand.
Researchers from the J-GEM collaboration observed a kilonova explosion, a phenomenon predicted to create heavy elements through rapid neutron capture reactions. The first-ever confirmed kilonova was detected using a network of telescopes worldwide, providing insight into the universe's heavy element production.
A team of Australian researchers has confirmed the detection of radio waves from a gravitational wave event, providing new insights into massive bodies like black holes. The discovery was made using the CSIRO's Australia Telescope Compact Array and marks a significant contribution to the global discovery of gravitational waves.
UCSB astronomers capture the fleeting kilonova using a network of telescopes and gravitational wave data. The event sheds light on the formation of heavy elements in the universe.
For the first time, scientists have detected both gravitational waves and electromagnetic radiation from the merger of two neutron stars, creating a new black hole. The detection marks the beginning of a new era in multi-messenger space exploration.
The LIGO-Virgo Collaboration observed the merger of two neutron stars, producing gravitational waves and a gamma-ray burst, marking the birth of multi-messenger astronomy. This discovery confirms kilonova formation, providing insight into the universe's heaviest elements.
Astronomers have made the first-ever observations of a merging neutron star, detecting both gravitational waves and a brilliant explosion of visible light. The discovery has opened a new window into understanding neutron star physics and could resolve a long-standing question about the origins of heavy elements.
RIT researchers played a significant role in the groundbreaking detection of colliding neutron stars by LIGO. This event marked the first time both gravitational waves and light were detected from the same cosmic collision.
The VLA detection and ongoing observations reveal key facts about the event that generated gravitational waves, including the amount of energy released and the environment in which it occurred. Radio waves will continue to provide valuable information for months or even years.
Scientists at Tel Aviv University utilize Nobel-winning research to detect gravitational waves produced by the merger of two ancient neutron stars. This discovery combines gravitational waves with light, producing a detailed model of the emission for the first time.
Researchers confirm neutron star collision using electromagnetic radiation detected by NASA's Swift Gamma Ray Burst Explorer. The event provided a complete picture of compact object mergers, marking a major breakthrough in astronomy.
Scientists at Oregon State University predicted a short gamma-ray burst detection, which was confirmed just a month later. The OSU team predicted the event based on their understanding of binary neutron star systems and gravitational waves.
Astronomers have observed a neutron star merger, detecting gravitational waves and gamma-ray signatures. Computer simulations suggest that the merger produces heavy elements, which are then dispersed into space, potentially seeding the universe with gold, platinum, and other rare elements.
A team of scientists from around the world detected gravitational waves and visible light from the collision of two neutron stars. The discovery marks a new era in multimessenger astronomy, allowing researchers to learn more about the universe through different kinds of electromagnetic radiation and gravitational waves.
Three GW astrophysicists contribute to global effort identifying kilonova explosion, a rare event roughly 1,000 times brighter than a nova. The discovery confirms predictions of gravitational waves and electromagnetic radiation from neutron-star mergers, providing insights into the formation and expansion of our universe.
The Columbia team will use machine learning and advanced techniques to filter out extraneous data and aid in the detection of gravitational waves. With a $1 million NSF grant, they aim to contribute to LIGO's historic breakthroughs and advance understanding of the cosmos.
The LIGO team detected gravitational waves from colliding black holes, providing a new way to explore the cosmos. Advanced optical interferometers enabled these breakthroughs, allowing scientists to study powerful astrophysical events.
The LIGO and Virgo Scientific Collaborations have detected a fourth gravitational wave signal, confirming Einstein's theory of general relativity. The detection was made using advanced optical interferometers and marks the first time three observatories have witnessed a merger at once.
The LIGO and Virgo observatories have jointly detected a black hole collision, emitting ripples in space and time. The event, located 1.8 billion light-years away, resulted in a spinning black hole with about 53 times the mass of our sun.
RIT researchers, in collaboration with LIGO and Virgo, successfully triangulated the position of a 1.8 billion-year-old black hole merger. With three advanced detectors observing together, scientists can now pinpoint locations with higher precision, enabling more accurate electromagnetic counterparts searches.
For the first time, three detectors tracked gravitational waves emitted by a merger of two black holes, allowing scientists to more closely locate their birthplace in space. The detection highlights the scientific potential of a three-detector network of gravitational-wave detectors.
Astronomers have detected the closest ever binary supermassive black hole system in galaxy NGC 7674, featuring two massive black holes with a combined mass of 40 million solar masses. The discovery is significant as it confirms theoretical predictions and provides insight into gravitational wave sources.
Researchers suggest black holes seen via gravitational waves spin slowly or rapidly, with tumbling behavior in dense environments; these findings provide new target for understanding black hole formation.
Researchers have discovered two detached, eclipsing double white dwarf binaries with orbital periods under an hour, producing significant gravitational waves. One binary is believed to be a new verification source for the Laser Interferometer Space Antenna, a gravitational wave satellite.
PIPER aims to detect primordial gravitational waves and study their effects on the cosmic microwave background, providing insight into the early universe's expansion. The mission will fly immersed in liquid helium at nearly absolute zero temperature.
Researchers from University of California, Irvine estimate tens of millions of stellar-remnant black holes exist in the Milky Way galaxy. The number of black holes is expected to depend on the size of the galaxy.
Rochester Institute of Technology (RIT) boasts the largest number of federally funded summer research programs for undergraduate students in New York. The institution's College of Science has launched several innovative research experiences, including a new program in multimessenger astrophysics that combines gravitational wave detecti...
Researchers suggest that massive star explosions can expel newborn black holes with strong natal kicks, affecting their spin and alignment. This phenomenon could help explain years of tentative evidence suggesting black holes receive such kicks.
Researchers suggest dense star clusters as source of gravitational waves, with black holes colliding to produce these waves. Computer simulations and observations point to globular clusters as ideal environments for black hole collisions.
The Laser Interferometer Gravitational-wave Observatory (LIGO) has confirmed the third detection of gravitational waves, revealing a population of black holes that were previously unknown. The detected black holes have masses ranging from 21 to 49 times that of the sun, shedding light on the existence of heavy black hole pairs.
Physicists at the University of Maryland contribute to the detection of a third gravitational wave event, GW170104, using data from Advanced LIGO detectors. The merger occurred approximately 3 billion years ago and produced a single, more massive black hole.
An international team of researchers detected gravitational waves from a binary black hole system, providing evidence that black holes in binary systems may not be aligned. The discovery highlights the need for further improvements in detector sensitivity to explore the universe.
Researchers at Rochester Institute of Technology contributed to the measurement of a newly discovered black hole's tilt and spin, which can reveal clues about how massive stars die. The findings support Einstein's general theory of relativity and rule out extreme predictions for black hole spins.
LIGO has made its third detection of gravitational waves, revealing a new population of black holes with masses up to 49 times that of the sun. The detected black holes were formed by merging pairs and provide clues about their spin directions, which may be non-aligned compared to their orbital motion.
Researchers at Monash University have identified a new concept called 'orphan memory,' which challenges current understanding of gravitational waves. They found that high-frequency waves leave behind a signature that LIGO can detect.
A team of NASA scientists is using LISA Pathfinder's advanced technology to map the distribution of tiny dust particles in space. By analyzing the spacecraft's response to microscopic dust impacts, they aim to refine models used in various studies, including planet formation and impact risks for spacecraft.
Astrophysicists at the University of Birmingham made progress in understanding how two black holes can merge, using Advanced LIGO data. The team found that all three observed events can be formed via isolated binary evolution via a common-envelope phase.
Astronomers discovered a supermassive black hole weighing over 1 billion suns that was propelled out of the center of a distant galaxy due to gravitational wave energy. The estimated equivalent energy is 100 million supernovas, and the black hole travels at speeds of up to 4.7 million miles per hour.
Caltech's Stan Whitcomb, a key figure in LIGO's development, will share insights into the project's groundbreaking discovery. He'll discuss how the detection confirmed Einstein's general theory of relativity and opened up new avenues for astronomy. The talk also touches on the technical challenges faced by LIGO detectors.
Researchers have made significant progress in developing stable laser sources for third-generation gravitational wave detectors, enabling the detection of weaker signals from distant cosmic events. The development includes a new type of pre-mode cleaner that compensates for astigmatism, making designs like the Einstein Telescope possible.
Theoretical physicists at the University of Basel have calculated the signal of specific gravitational wave sources that emerged fractions of a second after the Big Bang. These oscillons, predicted by Einstein, can be used to study the universe's early stages and provide information on major astrophysical events.
A new study suggests that determining the speed of gravity in the cosmos from gravitational waves could resolve the puzzle. If gravitational waves are found to travel at the speed of light, it would rule out alternative gravity theories and support Einstein's Cosmological Constant.
LIGO researcher Gabriela González has received the National Academy of Sciences Award for Scientific Discovery for her work on gravitational wave astronomy. She shares the award with David Howard Reitze and Peter R. Saulson, who have also contributed significantly to the field over 19 years.
Gabriela González, a professor at LSU and LIGO scientist, receives the 2017 Rossi Prize for her groundbreaking work on gravitational waves. Her discoveries have opened a new era in gravitational-wave astronomy.
A study by Professors Bhattacharyya and Chakrabarty suggests that a population of neutron stars may emit gravitational waves continuously, which could slow down their spin rates. This finding has strong implications for the study of these dense objects in the universe.
A new magnetic mirror-based device has been developed to map radiation from shortly after the Big Bang, shedding light on gravitational waves and the early universe. The device can modulate polarization across a wide range of microwave frequencies, overcoming a major challenge in detecting B-mode polarization.
The LIGO Scientific Collaboration detected gravitational waves that could have been caused by the collision of two black holes. Researchers used theoretical models to test whether these signals could also be produced by gravastars, hypothetical objects proposed as an alternative to black holes.
Four Penn State researchers have been awarded a total of $450,000 by the Charles E. Kaufman Foundation to study RNA and its processes, as well as real-time gravitational wave detection. The research aims to advance methods for determining RNA structure in living cells and improve prospects for multi-messenger astrophysics.
The winners of the 2016 Kavli Prize in Astrophysics reveal their 40-year journey to detect gravitational waves. They share their insights on the challenges and breakthroughs in eavesdropping on space-time ripples, which have captured the world's imagination.
Rochester Institute of Technology professors Carlos Lousto and Manuela Campanelli have won separate grants worth $600,000 and $435,000 to advance gravitational wave astronomy. The funding will support research on black hole mergers and develop software tools for computational astrophysics.
Researchers develop new method to detect and measure black hole superkicks using gravitational waves, which occur when two spinning supermassive black holes collide. eLISA space-based detector expected to detect several runaway black holes upon launch in 2034.
Researchers at RIT create a faster and more accurate way to assess gravitational wave signals, inferring the sources that made them. They use numerical simulations of binary black holes to extract information directly from the data, improving accuracy over previous approximations.
Scientists using cosmological simulations and gravitational wave signals predict initial mass of supermassive black hole seeds. The research aims to uncover mechanism that created these massive black holes and when they formed in the early Universe.
Researchers have developed a new squeezed vacuum source that can reduce phase noise in laser interferometers, enabling the detection of weaker gravitational waves. This advancement could enable the observation of more faint signals from distant events, including neutron star collisions.
A new study in Nature predicts hundreds of massive black hole mergers each year observable with the second generation of gravitational wave detectors. The model takes into account differences in binary black hole production across the universe.