scholarly journals The current status of binary black hole simulations in numerical relativity

2010 ◽  
Vol 27 (11) ◽  
pp. 114004 ◽  
Author(s):  
Ian Hinder
2015 ◽  
Vol 115 (12) ◽  
Author(s):  
Jonathan Blackman ◽  
Scott E. Field ◽  
Chad R. Galley ◽  
Béla Szilágyi ◽  
Mark A. Scheel ◽  
...  

Author(s):  
Sarah Habib ◽  
Antoni Ramos-Buades ◽  
Eliu Huerta ◽  
Sascha Husa ◽  
Roland Haas ◽  
...  

2017 ◽  
Vol 95 (10) ◽  
Author(s):  
Jonathan Blackman ◽  
Scott E. Field ◽  
Mark A. Scheel ◽  
Chad R. Galley ◽  
Daniel A. Hemberger ◽  
...  

2008 ◽  
Vol 25 (11) ◽  
pp. 114047 ◽  
Author(s):  
Deirdre Shoemaker ◽  
Birjoo Vaishnav ◽  
Ian Hinder ◽  
Frank Herrmann

2014 ◽  
Vol 89 (4) ◽  
Author(s):  
Prayush Kumar ◽  
Ilana MacDonald ◽  
Duncan A. Brown ◽  
Harald P. Pfeiffer ◽  
Kipp Cannon ◽  
...  

2021 ◽  
Vol 24 (1) ◽  
Author(s):  
Koutarou Kyutoku ◽  
Masaru Shibata ◽  
Keisuke Taniguchi

AbstractWe review the current status of general relativistic studies for coalescences of black hole–neutron star binaries. First, high-precision computations of black hole–neutron star binaries in quasiequilibrium circular orbits are summarized, focusing on the quasiequilibrium sequences and the mass-shedding limit. Next, the current status of numerical-relativity simulations for the merger of black hole–neutron star binaries is described. We summarize our understanding for the merger process, tidal disruption and its criterion, properties of the merger remnant and ejected material, gravitational waveforms, and gravitational-wave spectra. We also discuss expected electromagnetic counterparts to black hole–neutron star coalescences.


2019 ◽  
Vol 100 (6) ◽  
Author(s):  
E. A. Huerta ◽  
Roland Haas ◽  
Sarah Habib ◽  
Anushri Gupta ◽  
Adam Rebei ◽  
...  

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