Primordial Black Holes from Long-Range Scalar Forces and Scalar Radiative Cooling

Flores, Marcos M.; Kusenko, Alexander

doi:10.1103/physrevlett.126.041101

Title: Primordial Black Holes from Long-Range Scalar Forces and Scalar Radiative Cooling

Journal Article · Tue Jan 26 00:00:00 EST 2021 · Physical Review Letters

DOI:https://doi.org/10.1103/physrevlett.126.041101· OSTI ID:1836643

^[1]; Kusenko, Alexander ^[2]

Univ. of California, Los Angeles, CA (United States)
Univ. of California, Los Angeles, CA (United States); Univ. of Tokyo (Japan). Kavli Institute for the Physics and Mathematics of the Universe (WPI); Univ. of Tokyo (Japan)

We describe a new scenario for the formation of primordial black holes (PBHs). In the early Universe, the long-range forces mediated by the scalar fields can lead to formation of halos of heavy particles even during the radiation-dominated era. The same interactions result in the emission of scalar radiation from the motion and close encounters of particles in such halos. Radiative cooling due the scalar radiation allows the halos to collapse to black holes. We illustrate this scenario on a simple model with fermions interacting via the Yukawa forces. The abundance and the mass function of PBHs are suitable to account for all dark matter, or for some gravitational wave events detected by LIGO. The model relates the mass of the dark-sector particles to the masses and abundance of dark matter PBHs in a way that can explain why the dark matter and the ordinary matter have similar mass densities. The model also predicts a small contribution to the number of effective light degrees of freedom, which can help reconcile different measurements of the Hubble constant.

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Research Organization:: Univ. of California, Los Angeles, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP); USDOE Office of Science (SC) High Energy Physics (HEP)

Grant/Contract Number:: SC0009937

OSTI ID:: 1836643

Alternate ID(s):: OSTI ID: 1905677

Journal Information:: Physical Review Letters, Vol. 126, Issue 4; ISSN 0031-9007

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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