scholarly journals Astroseismology of neutron stars from gravitational waves in the limit of perfect measurement

2018 ◽  
Vol 478 (1) ◽  
pp. 167-171 ◽  
Author(s):  
A G Suvorov
Keyword(s):  
Neutron Stars ◽  
Gravitational Waves

scholarly journals Probing the internal composition of neutron stars with gravitational waves

2015 ◽  
Vol 92 (10) ◽  
Author(s):  
Katerina Chatziioannou ◽  
Kent Yagi ◽  
Antoine Klein ◽  
Neil Cornish ◽  
Nicolás Yunes
Keyword(s):  
Neutron Stars ◽  
Gravitational Waves

scholarly journals Gravitational Waves from Accreting Neutron Stars Undergoing Common-envelope Inspiral

2018 ◽  
Vol 857 (1) ◽  
pp. 38 ◽  
Author(s):  
A. Miguel Holgado ◽  
Paul M. Ricker ◽  
E. A. Huerta
Keyword(s):  
Neutron Stars ◽  
Gravitational Waves ◽  
Common Envelope

scholarly journals Gravitational Waves and Tidal Deformability of Neutron Stars

2018 ◽  
Vol 68 (7) ◽  
pp. 707-717
Author(s):  
Young-Min KIM ◽  
Kyujin KWAK ◽  
Yeunhwan LIM ◽  
Chang Ho HYUN ◽  
Chang-Hwan LEE*
Keyword(s):  
Neutron Stars ◽  
Gravitational Waves

LIGO/Virgo Listens to Neutron Stars

2020 ◽  
pp. 137-145
Author(s):  
John W. Moffat
Keyword(s):  
Neutron Star ◽  
Neutron Stars ◽  
Gravitational Waves ◽  
Gamma Ray ◽  
Accurate Determination ◽  
Hubble Constant ◽  
Gravitational Theory ◽  
Optical Signal ◽  
Gravity Models ◽  
Expansion Of The Universe

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.

scholarly journals Observational Limit on Gravitational Waves from Binary Neutron Stars in the Galaxy

1999 ◽  
Vol 83 (8) ◽  
pp. 1498-1501 ◽  
Author(s):  
B. Allen ◽  
J. K. Blackburn ◽  
P. R. Brady ◽  
J. D. E Creighton ◽  
T. Creighton ◽  
...  
Keyword(s):  
Neutron Stars ◽  
Gravitational Waves ◽  
The Galaxy ◽  
Binary Neutron Stars
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