Coalescence of Spinning Binary Neutron Stars of Equal Mass: 3D Numerical Simulations-Reference-Cited by-同舟云学术

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Coalescence of Spinning Binary Neutron Stars of Equal Mass: 3D Numerical Simulations

Published:1992-12-01 Issue:6 Volume:88 Page:1079-1095
ISSN:0033-068X
Container-title:Progress of Theoretical Physics
language:en
Short-container-title:Progress of Theoretical Physics

Author:

Shibata M.,Nakamura T.,Oohara K.-i.

Publisher

Oxford University Press (OUP)

Subject

Physics and Astronomy (miscellaneous)

Link

http://academic.oup.com/ptp/article-pdf/88/6/1079/5248120/88-6-1079.pdf

Reference1 articles.

1. Post-Newtonian hydrodynamics and post-Newtonian gravitational wave generation for numerical relativity

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1. Multimessenger Binary Mergers Containing Neutron Stars: Gravitational Waves, Jets, and γ-Ray Bursts;Frontiers in Astronomy and Space Sciences;2021-04-08

2. Impact of GW170817 for the nuclear physics of the EOS and the r-process;Annals of Physics;2019-12

3. Numerical relativity of compact binaries in the 21st century;Reports on Progress in Physics;2018-11-07

4. Binary Neutron Star Mergers;Living Reviews in Relativity;2012-07-04

5. Formation of black hole and emission of gravitational waves;Proceedings of the Japan Academy, Series B;2006

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