. | . |
LIGO-Virgo-KAGRA collaboration announces 90 gravitational wave discoveries to date by Staff Writers Rochester NY (SPX) Nov 09, 2021
The LIGO-Virgo-KAGRA Collaboration unveiled several studies that shed important new light on the nature of gravitational waves-ripples in time and space produced by merging black holes and/or neutron stars. They include a "census" of gravitational wave events to date and a new catalog of results from the second half of its third observing run (O3b), describing 90 gravitational wave events observed since making their first detection in 2015. Students and faculty from Rochester Institute of Technology's Center for Computational Relativity and Gravitation (CCRG) were heavily involved in analyzing the gravitational waves and understanding their significance. The catalog revealed 35 new events, including 32 black hole mergers and at least two black hole-neutron star mergers. Several of the resulting black holes that formed from these mergers exceed 100 times the mass of our sun and are classified as intermediate-mass black holes, which have long been theorized by astrophysicists. These most recent LIGO-Virgo-KAGRA observations confirm that this new class of black holes is more common in the universe than previously thought. Anjali Yelikar, an astrophysical sciences and technology Ph.D. student from India, contributed heavily to the study by using parameter estimation code to find the mass, spin, distance from Earth, and position in the sky of the black holes and neutron stars detected. She said being part of these discoveries as they happen at an increasingly rapid rate has been exhilarating. "It's fascinating because it's still such a young field," said Yelikar. "This is a new way to look at the universe. When I was younger, the Hubble Space Telescope was the cutting edge, but now we have developed these detectors that are so big, so sensitive that we are achieving levels that we could never have dreamed of." Associate Professor Richard O'Shaughnessy, who made key contributions to the paper outlining the population properties of mergers recorded to date, said, "We now have a better census of the universe and found some really interesting things in the second half of the last observing run. Now that we have observed so many events, we can understand more subtle properties of the population." O'Shaughnessy said that by studying 74 of the events detected by LIGO with the highest degree of confidence, they identified several important takeaways. First, the collaboration is able to estimate the merger rate for every type of event observed with the same framework for all. Second, the masses of the neutron stars detected by LIGO are significantly different from those observed previously within our own galaxy. And third, mergers seem to be happening far more frequently at certain masses, which have important astrophysical implications but needs to be confirmed with more sensitive future observing runs. The LIGO and Virgo observatories are currently undergoing improvements before the upcoming fourth observing run, expected to begin in the latter half of 2022. The KAGRA observatory in Japan will also join the next full observing run. Located deep under a mountain, KAGRA completed a successful first observing run in 2020 but has yet to join LIGO and Virgo in making joint observations. With more detectors, potential events can be located more accurately. RIT has an extensive group of students, faculty, postdoctoral researchers, and alumni involved in the LIGO Scientific Collaboratio
Research Report: The population of merging compact binaries inferred using gravitational waves through GWTC-3
Gravitational 'kick' may explain the strange shape at the center of Andromeda Boulder CO (SPX) Nov 03, 2021 When two galaxies collide, the supermassive black holes at their cores release a devastating gravitational "kick," similar to the recoil from a shotgun. New research led by CU Boulder suggests that this kick may be so powerful it can knock millions of stars into wonky orbits. The research, published Oct. 29 in The Astrophysical Journal Letters, helps solve a decades-old mystery surrounding a strangely-shaped cluster of stars at the heart of the Andromeda Galaxy. It might also help researchers bett ... read more
|
|
The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us. |