Dynamical evolution of black hole-neutron star binaries in general relativity: Simulations of tidal disruption

2006 ◽  
Vol 73 (2) ◽  
Author(s):  
Joshua A. Faber ◽  
Thomas W. Baumgarte ◽  
Stuart L. Shapiro ◽  
Keisuke Taniguchi ◽  
Frederic A. Rasio
2008 ◽  
Author(s):  
Masaru Shibata ◽  
Keisuke Taniguchi ◽  
Koji Uryū ◽  
Ye-Fei Yuan ◽  
Xiang-Dong Li ◽  
...  

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.


2004 ◽  
Vol 70 (6) ◽  
Author(s):  
Thomas W. Baumgarte ◽  
Monica L. Skoge ◽  
Stuart L. Shapiro

2008 ◽  
Vol 78 (10) ◽  
Author(s):  
Matthew D. Duez ◽  
Francois Foucart ◽  
Lawrence E. Kidder ◽  
Harald P. Pfeiffer ◽  
Mark A. Scheel ◽  
...  

2005 ◽  
Vol 72 (4) ◽  
Author(s):  
Keisuke Taniguchi ◽  
Thomas W. Baumgarte ◽  
Joshua A. Faber ◽  
Stuart L. Shapiro

2006 ◽  
Vol 74 (4) ◽  
Author(s):  
Keisuke Taniguchi ◽  
Thomas W. Baumgarte ◽  
Joshua A. Faber ◽  
Stuart L. Shapiro

2021 ◽  
Vol 912 (1) ◽  
pp. L18
Author(s):  
William E. East ◽  
Luis Lehner ◽  
Steven L. Liebling ◽  
Carlos Palenzuela

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