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Spectrum of a radio pulse from an exploding black hole

Blandford, R. D. (1977) Spectrum of a radio pulse from an exploding black hole. Monthly Notices of the Royal Astronomical Society, 181 (3). pp. 489-498. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20190521-165453560

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Abstract

Black holes of mass ≲ 10^(11) kg may be able to radiate all of their rest mass in an essentially instantaneous explosion by the Hawking process provided that the number of available modes increases sufficiently rapidly with temperature. Rees has pointed out that should this happen, electron–positron pairs may form a significant fraction of the explosion products and that if the hole is surrounded by a typical interstellar magnetic field, the kinetic energy of the pairs may be efficiently transformed into radio waves. In this paper the spectrum of the observed radiation is calculated and conditions necessary for this to be detectable are further discussed.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/181.3.489DOIArticle
http://adsabs.harvard.edu/abs/1977MNRAS.181..489BADSArticle
ORCID:
AuthorORCID
Blandford, R. D.0000-0002-1854-5506
Additional Information:© 1977 Royal Astronomical Society. Provided by the NASA Astrophysics Data System. Received 1977 May 26. I thank M. Rees for suggesting this problem, C. Alcock and D. Mikkelsen for numerical evaluation of the integral in Section 4 and J. Arons, C. McKee, A. Moffett and P. Young for helpful comments. This work was supported in part by the National Science Foundation (AST76-80801).
Group:TAPIR
Funders:
Funding AgencyGrant Number
NSFAST76-80801
Issue or Number:3
Record Number:CaltechAUTHORS:20190521-165453560
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190521-165453560
Official Citation:R. D. Blandford, Spectrum of a radio pulse from an exploding black hole, Monthly Notices of the Royal Astronomical Society, Volume 181, Issue 3, 1 December 1977, Pages 489–498, https://doi.org/10.1093/mnras/181.3.489
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95670
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:23 May 2019 18:10
Last Modified:03 Oct 2019 21:15

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