scholarly journals Model of the stochastic gravitational-wave background due to core collapse to black holes

2015 ◽  
Vol 92 (6) ◽  
Author(s):  
K. Crocker ◽  
V. Mandic ◽  
T. Regimbau ◽  
K. Belczynski ◽  
W. Gladysz ◽  
...  
Keyword(s):  
Black Holes ◽  
Gravitational Wave ◽  
Core Collapse ◽  
Gravitational Wave Background

scholarly journals GW150914: Implications for the Stochastic Gravitational-Wave Background from Binary Black Holes

2016 ◽  
Vol 116 (13) ◽  
Author(s):  
B. P. Abbott ◽  
R. Abbott ◽  
T. D. Abbott ◽  
M. R. Abernathy ◽  
F. Acernese ◽  
...  
Keyword(s):  
Black Holes ◽  
Gravitational Wave ◽  
Binary Black Holes ◽  
Gravitational Wave Background

Dynamical versus isolated formation channels of gravitational wave sources

2018 ◽  
Vol 14 (S346) ◽  
pp. 397-416
Author(s):  
Michela Mapelli
Keyword(s):  
Black Holes ◽  
Neutron Stars ◽  
Gravitational Wave ◽  
Theoretical Models ◽  
Stellar Winds ◽  
Core Collapse ◽  
Dynamical Processes ◽  
New Approach ◽  
The Impact

AbstractWhat are the formation channels of merging black holes and neutron stars? The first two observing runs of Advanced LIGO and Virgo give us invaluable insights to address this question, but a new approach to theoretical models is required, in order to match the challenges posed by the new data. In this review, I discuss the impact of stellar winds, core-collapse and pair instability supernovae on the formation of compact remnants in both isolated and dynamically formed binaries. Finally, I show that dynamical processes, such as the runaway collision scenario and the Kozai-Lidov mechanism, leave a clear imprint on the demography of merging systems.

scholarly journals Metallicity-constrained merger rates of binary black holes and the stochastic gravitational wave background

2016 ◽  
Vol 461 (4) ◽  
pp. 3877-3885 ◽  
Author(s):  
Irina Dvorkin ◽  
Elisabeth Vangioni ◽  
Joseph Silk ◽  
Jean-Philippe Uzan ◽  
Keith A. Olive
Keyword(s):  
Black Holes ◽  
Gravitational Wave ◽  
Binary Black Holes ◽  
Gravitational Wave Background
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