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The Shadow of the Black Hole$
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John W. Moffat

Print publication date: 2020

Print ISBN-13: 9780190650728

Published to Oxford Scholarship Online: June 2020

DOI: 10.1093/oso/9780190650728.001.0001

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PRINTED FROM OXFORD SCHOLARSHIP ONLINE (oxford.universitypressscholarship.com). (c) Copyright Oxford University Press, 2021. All Rights Reserved. An individual user may print out a PDF of a single chapter of a monograph in OSO for personal use. date: 28 September 2021

LIGO/Virgo Listens to Neutron Stars

LIGO/Virgo Listens to Neutron Stars

Chapter:
(p.137) 8 LIGO/Virgo Listens to Neutron Stars
Source:
The Shadow of the Black Hole
Author(s):

John W. Moffat

Publisher:
Oxford University Press
DOI:10.1093/oso/9780190650728.003.0008

On August 8, 2017, LIGO/Virgo detected the merging of two neutron stars 130 million light years away. Just 1.7 seconds later, the Fermi Gamma Ray Space Telescope received an optical signal—a short gamma ray burst (GRB). Thus began a new era of “multimessenger astronomy.” The GRBs are very energetic explosions observed in galaxies. The neutron star merger offers the first evidence that heavy metals such as gold, platinum, and uranium were created by the collision of neutron stars in a “kilonova.” The resulting gravitational waves offer a new way of measuring the Hubble constant, which determines the rate of expansion of the universe. An important result from the neutron star merger is an extremely accurate determination of the speed of gravitational waves; they move at the speed of light. This has significant ramifications for gravitational theory. It falsifies many proposed modified gravity models.

Keywords:   neutron star merger, LIGO/Virgo observatory, multimessenger astronomy, gamma ray burst, kilonova, Hubble constant

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