Notes on primordial black hole origin for thermal gamma-ray bursts

Author:

McMaken Tyler1ORCID

Affiliation:

1. JILA and Department of Physics, University of Colorado, Boulder, CO 80309, USA

Abstract

ABSTRACT Recently, an alleged plausible astrophysical scenario was proposed for the production of observed thermal gamma-ray bursts, via Hawking radiation emitted from a primordial black hole (PBH) freely falling into a more massive black hole. Here, the implausibility of that scenario is demonstrated, and the key flaws in that paper’s calculations and assumptions are elucidated through a discussion of some common misconceptions concerning black holes and general relativity. In particular, the predicted radiance observed from Earth is found to be orders of magnitude lower than what any instrument could detect, and the PBH–BH merger signature would be completely overwhelmed by the background Hawking signature from free PBHs.

Funder

JILA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Gamma-ray emission from primordial black hole–neutron star interaction;Monthly Notices of the Royal Astronomical Society;2022-08-25

2. Erratum: Primordial black hole origin for thermal gamma-ray bursts;Monthly Notices of the Royal Astronomical Society;2022-03-30

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