scholarly journals Gravitational-wave Detection and Parameter Estimation for Accreting Black-hole Binaries and Their Electromagnetic Counterpart

2020 ◽  
Vol 892 (2) ◽  
pp. 90 ◽  
Author(s):  
Andrea Caputo ◽  
Laura Sberna ◽  
Alexandre Toubiana ◽  
Stanislav Babak ◽  
Enrico Barausse ◽  
...  
Keyword(s):  
Black Hole ◽  
Parameter Estimation ◽  
Gravitational Wave ◽  
Gravitational Wave Detection ◽  
Black Hole Binaries ◽  
Wave Detection

scholarly journals On the Rarity of Double Black Hole Binaries: Consequences for Gravitational Wave Detection

2007 ◽  
Vol 662 (1) ◽  
pp. 504-511 ◽  
Author(s):  
Krzysztof Belczynski ◽  
Ronald E. Taam ◽  
Vassiliki Kalogera ◽  
Frederic A. Rasio ◽  
Tomasz Bulik
Keyword(s):  
Black Hole ◽  
Gravitational Wave ◽  
Gravitational Wave Detection ◽  
Black Hole Binaries ◽  
Wave Detection

scholarly journals THE FORMATION AND GRAVITATIONAL-WAVE DETECTION OF MASSIVE STELLAR BLACK HOLE BINARIES

2014 ◽  
Vol 789 (2) ◽  
pp. 120 ◽  
Author(s):  
Krzysztof Belczynski ◽  
Alessandra Buonanno ◽  
Matteo Cantiello ◽  
Chris L. Fryer ◽  
Daniel E. Holz ◽  
...  
Keyword(s):  
Black Hole ◽  
Gravitational Wave ◽  
Gravitational Wave Detection ◽  
Black Hole Binaries ◽  
Wave Detection

scholarly journals Samurai project: Verifying the consistency of black-hole-binary waveforms for gravitational-wave detection

2009 ◽  
Vol 79 (8) ◽  
Author(s):  
Mark Hannam ◽  
Sascha Husa ◽  
John G. Baker ◽  
Michael Boyle ◽  
Bernd Brügmann ◽  
...  
Keyword(s):  
Black Hole ◽  
Gravitational Wave ◽  
Gravitational Wave Detection ◽  
Wave Detection ◽  
Black Hole Binary

Gravitational waves from neutron star binaries

2017 ◽  
Vol 26 (01n02) ◽  
pp. 1740015 ◽  
Author(s):  
Chang-Hwan Lee
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Neutron Stars ◽  
Gravitational Wave ◽  
Gravitational Waves ◽  
Future Prospect ◽  
Black Hole Binaries ◽  
Wave Detection ◽  
Low Mass ◽  
Merger Rate

With H. A. Bethe, G. E. Brown worked on the merger rate of neutron star binaries for the gravitational wave detection. Their prediction has to be modified significantly due to the observations of [Formula: see text] neutron stars and the detection of gravitational waves. There still, however, remains a possibility that neutron star-low mass black hole binaries are significant sources of gravitational waves for the ground-based detectors. In this paper, I review the evolution of neutron star binaries with super-Eddington accretion and discuss the future prospect.

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