On mass distribution of coalescing black holes
Autor: | A. G. Kuranov, N.A. Mitichkin, Alexander D. Dolgov, O. S. Sazhina, I. V. Simkin, Konstantin Postnov, S. Porey |
---|---|
Rok vydání: | 2020 |
Předmět: |
Physics
Cosmology and Nongalactic Astrophysics (astro-ph.CO) Mass distribution 010308 nuclear & particles physics Astrophysics::High Energy Astrophysical Phenomena FOS: Physical sciences Astronomy and Astrophysics Astrophysics 01 natural sciences LIGO High Energy Physics - Phenomenology General Relativity and Quantum Cosmology High Energy Physics - Phenomenology (hep-ph) Binary black hole 0103 physical sciences Binary star Chirp Mass spectrum Range (statistics) Astrophysics - Cosmology and Nongalactic Astrophysics |
Zdroj: | Journal of Cosmology and Astroparticle Physics. 2020:017-017 |
ISSN: | 1475-7516 |
DOI: | 10.1088/1475-7516/2020/12/017 |
Popis: | Available data on the chirp mass distribution of the coalescing black hole binaries in O1-O3 LIGO/Virgo runs are analyzed and compared statistically with the distribution calculated under the assumption that these black holes are primordial with a log-normal mass spectrum. The theoretically calculated chirp mass distribution with the inferred best acceptable mass spectrum parameters, $M_0=17 M_\odot$ and $\gamma=0.9$, perfectly describes the data. The value of $M_0$ very well agrees with the theoretically expected one. On the opposite, the chirp mass distribution of black hole binaries originated from massive binary star evolution requires additional model adjustments to reproduce the observed chirp mass distribution Comment: 17 pages, 8 figures, one figure and reference added, revised version submitted to JCAP |
Databáze: | OpenAIRE |
Externí odkaz: |