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BlackHawk: a public code for calculating the Hawking evaporation spectra of any black hole distribution

We describe BlackHawk, a public C program for calculating the Hawking evaporation spectra of any black hole distribution. This program enables the users to compute the primary and secondary spectra of stable or long-lived particles generated by Hawking radiation of the distribution of black holes, a...

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Detalles Bibliográficos
Autores principales: Arbey, Alexandre, Auffinger, Jérémy
Lenguaje:eng
Publicado: 2019
Materias:
Acceso en línea:https://dx.doi.org/10.1140/epjc/s10052-019-7161-1
http://cds.cern.ch/record/2674326
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author Arbey, Alexandre
Auffinger, Jérémy
author_facet Arbey, Alexandre
Auffinger, Jérémy
author_sort Arbey, Alexandre
collection CERN
description We describe BlackHawk, a public C program for calculating the Hawking evaporation spectra of any black hole distribution. This program enables the users to compute the primary and secondary spectra of stable or long-lived particles generated by Hawking radiation of the distribution of black holes, and to study their evolution in time. The physics of Hawking radiation is presented, and the capabilities, features and usage of BlackHawk are described here under the form of a manual. The BlackHawk code can be downloaded from https://blackhawk.hepforge.org .
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2019
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spelling cern-26743262022-07-08T12:32:03Zdoi:10.1140/epjc/s10052-019-7161-1http://cds.cern.ch/record/2674326engArbey, AlexandreAuffinger, JérémyBlackHawk: a public code for calculating the Hawking evaporation spectra of any black hole distributionParticle Physics - PhenomenologyAstrophysics and AstronomyGeneral Relativity and CosmologyWe describe BlackHawk, a public C program for calculating the Hawking evaporation spectra of any black hole distribution. This program enables the users to compute the primary and secondary spectra of stable or long-lived particles generated by Hawking radiation of the distribution of black holes, and to study their evolution in time. The physics of Hawking radiation is presented, and the capabilities, features and usage of BlackHawk are described here under the form of a manual. The BlackHawk code can be downloaded from https://blackhawk.hepforge.org .We describe BlackHawk, a public C program for calculating the Hawking evaporation spectra of any black hole distribution. This program allows the users to compute the primary and secondary spectra of stable or long-lived particles generated by Hawking radiation of the distribution of black holes, and to study their evolution in time. The physics of Hawking radiation is presented, and the capabilities, features and usage of BlackHawk are described here under the form of a manual. This is the BlackHawk v2.0 manual, which is available on the BlackHawk webpage http://blackhawk.hepforge.org/. A brief release note summarizing the new aspects of BlackHawk v2.0 as well as illustrating examples can be found in https://arxiv.org/abs/2108.02737.arXiv:1905.04268CERN-TH-2019-067oai:cds.cern.ch:26743262019-05-10
spellingShingle Particle Physics - Phenomenology
Astrophysics and Astronomy
General Relativity and Cosmology
Arbey, Alexandre
Auffinger, Jérémy
BlackHawk: a public code for calculating the Hawking evaporation spectra of any black hole distribution
title BlackHawk: a public code for calculating the Hawking evaporation spectra of any black hole distribution
title_full BlackHawk: a public code for calculating the Hawking evaporation spectra of any black hole distribution
title_fullStr BlackHawk: a public code for calculating the Hawking evaporation spectra of any black hole distribution
title_full_unstemmed BlackHawk: a public code for calculating the Hawking evaporation spectra of any black hole distribution
title_short BlackHawk: a public code for calculating the Hawking evaporation spectra of any black hole distribution
title_sort blackhawk: a public code for calculating the hawking evaporation spectra of any black hole distribution
topic Particle Physics - Phenomenology
Astrophysics and Astronomy
General Relativity and Cosmology
url https://dx.doi.org/10.1140/epjc/s10052-019-7161-1
http://cds.cern.ch/record/2674326
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