Quasiequilibrium sequences of synchronously rotating binary neutron stars with constant rest masses in general relativity: Another approach without using the conformally flat condition

2002 ◽  
Vol 65 (6) ◽  
Author(s):  
Fumihiko Usui ◽  
Yoshiharu Eriguchi
2017 ◽  
Vol 2017 ◽  
pp. 1-12 ◽  
Author(s):  
In-Saeng Suh ◽  
Grant J. Mathews ◽  
J. Reese Haywood ◽  
N. Q. Lan

The spatially conformally flat approximation (CFA) is a viable method to deduce initial conditions for the subsequent evolution of binary neutron stars employing the full Einstein equations. Here we analyze the viability of the CFA for the general relativistic hydrodynamic initial conditions of binary neutron stars. We illustrate the stability of the conformally flat condition on the hydrodynamics by numerically evolving ~100 quasicircular orbits. We illustrate the use of this approximation for orbiting neutron stars in the quasicircular orbit approximation to demonstrate the equation of state dependence of these initial conditions and how they might affect the emergent gravitational wave frequency as the stars approach the innermost stable circular orbit.


2001 ◽  
Vol 63 (6) ◽  
Author(s):  
Eric Gourgoulhon ◽  
Philippe Grandclément ◽  
Keisuke Taniguchi ◽  
Jean-Alain Marck ◽  
Silvano Bonazzola

2002 ◽  
pp. 2299-2300
Author(s):  
K. TANIGUCHI ◽  
E. GOURGOULHON ◽  
P. GRANDCLÉMENT ◽  
J.-A. MARCK ◽  
S. BONAZZOLA

1997 ◽  
Vol 79 (7) ◽  
pp. 1182-1185 ◽  
Author(s):  
T. W. Baumgarte ◽  
G. B. Cook ◽  
M. A. Scheel ◽  
S. L. Shapiro ◽  
S. A. Teukolsky

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