scholarly journals New numerical method for constructing quasiequilibrium sequences of irrotational binary neutron stars in general relativity

2000 ◽  
Vol 61 (12) ◽  
Author(s):  
Kōji Uryū ◽  
Yoshiharu Eriguchi
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

2021 ◽  
Vol 30 (6) ◽  
pp. 7-13
Author(s):  
Jinho KIM

Compact stars, e.g., black holes and neutron stars, are the most energetic objects in astrophysics. These objects are accompanied by extremely strong gravity and a high velocity, which approaches the speed of light. Therefore, compact objects should be dealt with in Einstein’s relativity. This article will briefly introduce a numerical method that will allow us to obtain general solutions in general relativity. Several applications using numerical relativistic simulations will also be presented.


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