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

A. Dolgov; K. Postnov

doi:10.1088/1475-7516/2020/07/063

Why the mean mass of primordial black hole distribution is close to 10M_⊙

Результат исследования: Научные публикации в периодических изданиях › статья

Аннотация

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.

Язык оригинала	английский
Номер статьи	063
Журнал	Journal of Cosmology and Astroparticle Physics
Том	2020
Номер выпуска	7
DOI	https://doi.org/10.1088/1475-7516/2020/07/063
Состояние	Опубликовано - 30 июл 2020

Доступ к документу

10.1088/1475-7516/2020/07/063

Link to publication in Scopus

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Цитировать

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

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