期刊
NEW ASTRONOMY
卷 51, 期 -, 页码 122-127出版社
ELSEVIER
DOI: 10.1016/j.newast.2016.08.017
关键词
Gravitational waves; GW150914; Black holes; LIGO; MASTER
资金
- Development Programm of Lomonosov Moscow State University
- Moscow Union OPTICA
- Russian Science Foundation [16-12-00085]
- Russian Foundation of Fundamental Research [15-02-07875]
- Russian Science Foundation [16-12-00085] Funding Source: Russian Science Foundation
The Advanced LIGO observatory recently reported (Abbott et al., 2016a) the first direct detection of gravitational waves predicted by Einstein (1916). The detection of this event was predicted in 1997 on the basis of the Scenario Machine population synthesis calculations (Lipunov et al., 1997b) Now we discuss the parameters of binary black holes and event rates predicted by different scenarios of binary evolution. We give a simple explanation of the big difference between detected black hole masses and the mean black hole masses observed in of X-ray Nova systems. The proximity of the masses of the components of GW150914 is in good agreement with the observed initial mass ratio distribution in massive binary systems, as is used in Scenario Machine calculations for massive binaries. (C) 2016 Elsevier B.V. All rights reserved.
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