2022MNRAS.511.1218M


Query : 2022MNRAS.511.1218M

2022MNRAS.511.1218M - Mon. Not. R. Astron. Soc., 511, 1218-1223 (2022/March-3)

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

McMAKEN T.

Abstract (from CDS):

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.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): black hole physics - dark matter - black hole mergers - gamma-ray bursts

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 1007 1
2 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1261 1
3 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
4 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1928 2

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