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arXiv · astro-ph/9606179

Coalescence of Binary Neutron Stars

Ken-ichi Oohara·Takashi Namamura
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Abstract

The most important sources for laser-interferometric gravitational-wave detectors like LIGO or VIRGO are catastrophic events such as coalescence of a neutron-star binary. The final phase, or the last three milliseconds, of coalescence is considered. We describe results of numerical simulations of coalescing binary neutron stars using Newtonian and post-Newtonian hydrodynamics code and then discuss recent development of our 3D GR code.

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Ken-ichi Oohara, Takashi Namamura. 1996-06-29. Coalescence of Binary Neutron Stars. https://arxiv.org/abs/astro-ph/9606179

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