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Why the mean mass of primordial black hole distribution is close to 10M⊙. / Dolgov, A.; Postnov, K.

In: Journal of Cosmology and Astroparticle Physics, Vol. 2020, No. 7, 063, 30.07.2020.

Research output: Contribution to journal › Article › peer-review

Harvard

Dolgov, A & Postnov, K 2020, 'Why the mean mass of primordial black hole distribution is close to 10M⊙', Journal of Cosmology and Astroparticle Physics, vol. 2020, no. 7, 063. https://doi.org/10.1088/1475-7516/2020/07/063

APA

Dolgov, A., & Postnov, K. (2020). Why the mean mass of primordial black hole distribution is close to 10M⊙. Journal of Cosmology and Astroparticle Physics, 2020(7), [063]. https://doi.org/10.1088/1475-7516/2020/07/063

Vancouver

Dolgov A, Postnov K. Why the mean mass of primordial black hole distribution is close to 10M⊙. Journal of Cosmology and Astroparticle Physics. 2020 Jul 30;2020(7):063. doi: 10.1088/1475-7516/2020/07/063

Author

Dolgov, A. ; Postnov, K. / Why the mean mass of primordial black hole distribution is close to 10M⊙. In: Journal of Cosmology and Astroparticle Physics. 2020 ; Vol. 2020, No. 7.

BibTeX

@article{b719664bfe6e4758ae1ab87366b7e8d1,
title = "Why the mean mass of primordial black hole distribution is close to 10M⊙",
abstract = "It is shown that a mechanism of PBH formation from high-baryon bubbles with log-normal mass spectrum naturally leads to the central mass of the PBH distribution close to ten solar masses independently of the model details. This result is in good agreement with observations.",
keywords = "baryon asymmetry, cosmological phase transitions, primordial black holes, BARYOGENESIS",
author = "A. Dolgov and K. Postnov",
year = "2020",
month = jul,
day = "30",
doi = "10.1088/1475-7516/2020/07/063",
language = "English",
volume = "2020",
journal = "Journal of Cosmology and Astroparticle Physics",
issn = "1475-7516",
publisher = "IOP Publishing Ltd.",
number = "7",

}

RIS

TY - JOUR

T1 - Why the mean mass of primordial black hole distribution is close to 10M⊙

AU - Dolgov, A.

AU - Postnov, K.

PY - 2020/7/30

Y1 - 2020/7/30

N2 - It is shown that a mechanism of PBH formation from high-baryon bubbles with log-normal mass spectrum naturally leads to the central mass of the PBH distribution close to ten solar masses independently of the model details. This result is in good agreement with observations.

AB - It is shown that a mechanism of PBH formation from high-baryon bubbles with log-normal mass spectrum naturally leads to the central mass of the PBH distribution close to ten solar masses independently of the model details. This result is in good agreement with observations.

KW - baryon asymmetry

KW - cosmological phase transitions

KW - primordial black holes

KW - BARYOGENESIS

UR - http://www.scopus.com/inward/record.url?scp=85089844063&partnerID=8YFLogxK

U2 - 10.1088/1475-7516/2020/07/063

DO - 10.1088/1475-7516/2020/07/063

M3 - Article

AN - SCOPUS:85089844063

VL - 2020

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

SN - 1475-7516

IS - 7

M1 - 063

ER -

ID: 25292295