DMCA
Black hole binary formation in the expanding universe: Three body problem approximation (1998)
| Venue: | Phys. Rev |
| Citations: | 2 - 0 self |
BibTeX
@ARTICLE{Ioka98blackhole,
author = {Kunihito Ioka and Takeshi Chiba and Takahiro Tanaka and Takashi Nakamura},
title = {Black hole binary formation in the expanding universe: Three body problem approximation},
journal = {Phys. Rev},
year = {1998}
}
Share
 |
 |
 |
 |
||
OpenURL
Abstract
We study black hole MACHO binary formation through three-body interactions in the early universe at t ∼ 10 −5 s. The probability distribution functions of the eccentricity and the semimajor axis of binaries as well as of the coalescence time are obtained assuming that the black holes are randomly formed in space. We confirm that the previous order-of-magnitude estimate for the binary parameters is valid within ∼ 50 % error. We find that the coalescence rate of the black hole MACHO binaries is ∼ 5 × 10 −2 × 2 ±1 events/year/galaxy taking into consideration several possible factors which may affect this estimate. This suggests that the event rate of coalescing binary black holes will be at least several events per year within 15 Mpc. The first LIGO/VIRGO interferometers in 2001 will be able to verify whether the MACHOs are black holes or not.
Keyphrases
body problem approximation black hole binary formation black hole previous order-of-magnitude estimate event year galaxy early universe semimajor axis black hole macho binary three-body interaction coalescence time several event probability distribution function event rate black hole macho binary formation binary black hole coalescence rate first ligo virgo interferometer binary parameter consideration several possible factor
