Standard

Spins of black holes in coalescing compact binaries. / Postnov, K. A.; Kuranov, A. G.; Mitichkin, N. A.

в: Physics-Uspekhi, Том 62, № 11, 11.2019, стр. 1153-1161.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Postnov, KA, Kuranov, AG & Mitichkin, NA 2019, 'Spins of black holes in coalescing compact binaries', Physics-Uspekhi, Том. 62, № 11, стр. 1153-1161. https://doi.org/10.3367/UFNe.2019.04.038593

APA

Postnov, K. A., Kuranov, A. G., & Mitichkin, N. A. (2019). Spins of black holes in coalescing compact binaries. Physics-Uspekhi, 62(11), 1153-1161. https://doi.org/10.3367/UFNe.2019.04.038593

Vancouver

Postnov KA, Kuranov AG, Mitichkin NA. Spins of black holes in coalescing compact binaries. Physics-Uspekhi. 2019 нояб.;62(11):1153-1161. doi: 10.3367/UFNe.2019.04.038593

Author

Postnov, K. A. ; Kuranov, A. G. ; Mitichkin, N. A. / Spins of black holes in coalescing compact binaries. в: Physics-Uspekhi. 2019 ; Том 62, № 11. стр. 1153-1161.

BibTeX

@article{d704739dfab6455486bcd014e4765c90,
title = "Spins of black holes in coalescing compact binaries",
abstract = "Modern astrophysical methods for determining spins of rotating stellar-mass black holes in close binaries and of supermassive black holes in active galactic nuclei are briefly discussed. Effective spins of coalescing binary black holes derived from LIGO/Virgo gravitational wave observations are specially addressed. The effective spins of coalescing astrophysical binary black holes and black holes with neutron stars are calculated for two plausible models of black hole formation from stellar core collapses (without or with an additional fallback from the stellar envelope) taking the stellar metallicity and star formation rate evolution in the Universe into account. The calculated distributions are consistent with the reported LIGO/Virgo observations. Distributions of the effective spins expected in yet undiscovered neutron star-black hole binaries have been calculated. The effective spins of primordial coalescing stellar-mass black holes can reach a few percent due to the accretion spin-up in a cold external medium.",
author = "Postnov, {K. A.} and Kuranov, {A. G.} and Mitichkin, {N. A.}",
year = "2019",
month = nov,
doi = "10.3367/UFNe.2019.04.038593",
language = "English",
volume = "62",
pages = "1153--1161",
journal = "Physics-Uspekhi",
issn = "1063-7869",
publisher = "Turpion Ltd.",
number = "11",

}

RIS

TY - JOUR

T1 - Spins of black holes in coalescing compact binaries

AU - Postnov, K. A.

AU - Kuranov, A. G.

AU - Mitichkin, N. A.

PY - 2019/11

Y1 - 2019/11

N2 - Modern astrophysical methods for determining spins of rotating stellar-mass black holes in close binaries and of supermassive black holes in active galactic nuclei are briefly discussed. Effective spins of coalescing binary black holes derived from LIGO/Virgo gravitational wave observations are specially addressed. The effective spins of coalescing astrophysical binary black holes and black holes with neutron stars are calculated for two plausible models of black hole formation from stellar core collapses (without or with an additional fallback from the stellar envelope) taking the stellar metallicity and star formation rate evolution in the Universe into account. The calculated distributions are consistent with the reported LIGO/Virgo observations. Distributions of the effective spins expected in yet undiscovered neutron star-black hole binaries have been calculated. The effective spins of primordial coalescing stellar-mass black holes can reach a few percent due to the accretion spin-up in a cold external medium.

AB - Modern astrophysical methods for determining spins of rotating stellar-mass black holes in close binaries and of supermassive black holes in active galactic nuclei are briefly discussed. Effective spins of coalescing binary black holes derived from LIGO/Virgo gravitational wave observations are specially addressed. The effective spins of coalescing astrophysical binary black holes and black holes with neutron stars are calculated for two plausible models of black hole formation from stellar core collapses (without or with an additional fallback from the stellar envelope) taking the stellar metallicity and star formation rate evolution in the Universe into account. The calculated distributions are consistent with the reported LIGO/Virgo observations. Distributions of the effective spins expected in yet undiscovered neutron star-black hole binaries have been calculated. The effective spins of primordial coalescing stellar-mass black holes can reach a few percent due to the accretion spin-up in a cold external medium.

UR - http://www.scopus.com/inward/record.url?scp=85081644216&partnerID=8YFLogxK

U2 - 10.3367/UFNe.2019.04.038593

DO - 10.3367/UFNe.2019.04.038593

M3 - Article

AN - SCOPUS:85081644216

VL - 62

SP - 1153

EP - 1161

JO - Physics-Uspekhi

JF - Physics-Uspekhi

SN - 1063-7869

IS - 11

ER -

ID: 24027664