Journal
ASTROPHYSICAL JOURNAL
Volume 864, Issue 1, Pages -Publisher
IOP Publishing Ltd
DOI: 10.3847/1538-4357/aad6e2
Keywords
black hole physics; gravitational waves
Categories
Funding
- NSFC [11335012, 11575271, 11690021, 11747601]
- Top-Notch Young Talents Program of China
- Strategic Priority Research Program of CAS
- Key Research Program of Frontier Sciences of CAS
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Up to now several gravitational-wave events from the coalescences of black hole binaries have been reported by LIGO/VIRGO, and imply that black holes should have an extended mass function. We work out the merger rate distribution of primordial black hole (PBH) binaries with a general mass function by taking into account the torques by all PBHs and linear density perturbations. In the future, many more coalescences of black hole binaries are expected to be detected, and the one-dimensional and two-dimensional merger rate distributions will be crucial for reconstructing the mass function of PBHs.
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