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27 April 2024
 
  » arxiv » gr-qc/9704024

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Binary Neutron Stars in General Relativity: Quasi-Equilibrium Models
T. W. Baumgarte ; G. B. Cook ; M. A. Scheel ; S. L. Shapiro ; S. A. Teukolsky ;
Date 8 Apr 1997
Journal Phys.Rev.Lett. 79 (1997) 1182-1185
Subject gr-qc astro-ph
AbstractWe perform fully relativistic calculations of binary neutron stars in quasi-equilibrium circular orbits. We integrate Einstein’s equations together with the relativistic equation of hydrostatic equilibrium to solve the initial value problem for equal-mass binaries of arbitrary separation. We construct sequences of constant rest mass and identify the innermost stable circular orbit and its angular velocity. We find that the quasi-equilibrium maximum allowed mass of a neutron star in a close binary is slightly larger than in isolation.
Source arXiv, gr-qc/9704024
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