scholarly journals Black hole remnant of black hole-neutron star coalescing binaries with arbitrary black hole spin

2014 ◽  
Vol 89 (4) ◽  
Author(s):  
Francesco Pannarale
2009 ◽  
Vol 79 (4) ◽  
Author(s):  
Zachariah B. Etienne ◽  
Yuk Tung Liu ◽  
Stuart L. Shapiro ◽  
Thomas W. Baumgarte

2015 ◽  
Vol 92 (2) ◽  
Author(s):  
Kyohei Kawaguchi ◽  
Koutarou Kyutoku ◽  
Hiroyuki Nakano ◽  
Hirotada Okawa ◽  
Masaru Shibata ◽  
...  

2011 ◽  
Vol 83 (2) ◽  
Author(s):  
Francois Foucart ◽  
Matthew D. Duez ◽  
Lawrence E. Kidder ◽  
Saul A. Teukolsky

2014 ◽  
Vol 446 (1) ◽  
pp. 750-758 ◽  
Author(s):  
Rodrigo Fernández ◽  
Daniel Kasen ◽  
Brian D. Metzger ◽  
Eliot Quataert

2012 ◽  
Vol 85 (12) ◽  
Author(s):  
William E. East ◽  
Frans Pretorius ◽  
Branson C. Stephens

2021 ◽  
Vol 922 (1) ◽  
pp. L14
Author(s):  
Ilya Mandel ◽  
Rory J. E. Smith

Abstract GW200115 was the second merger of a black hole and a neutron star confidently detected through gravitational waves. Inference on the signal allows for a large black hole spin misaligned with the orbital angular momentum, but shows little support for aligned spin values. We show that this is a natural consequence of measuring the parameters of a black hole–neutron star binary with nonspinning components while assuming the priors used in the LIGO–Virgo–KAGRA analysis. We suggest that, a priori, a nonspinning binary is more consistent with current astrophysical understanding.


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