Total spectral distributions from Hawking radiation

Abstract Taking into account the time dependence of the Hawking temperature and finite evaporation time of the black hole, the total spectral distributions of the radiant energy and of the number of particles have been explicitly calculated and compared to their temporary (initial) blackbody counter...

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Main Author: Bogusław Broda
Format: Article
Language:English
Published: SpringerOpen 2017-11-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-017-5336-1
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spelling doaj-75eb2d14745b472bbab3bc9a53fa7e472020-11-24T22:25:28ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522017-11-0177111510.1140/epjc/s10052-017-5336-1Total spectral distributions from Hawking radiationBogusław Broda0Department of Theoretical Physics, Faculty of Physics and Applied Informatics, University of ŁódźAbstract Taking into account the time dependence of the Hawking temperature and finite evaporation time of the black hole, the total spectral distributions of the radiant energy and of the number of particles have been explicitly calculated and compared to their temporary (initial) blackbody counterparts (spectral exitances).http://link.springer.com/article/10.1140/epjc/s10052-017-5336-1
collection DOAJ
language English
format Article
sources DOAJ
author Bogusław Broda
spellingShingle Bogusław Broda
Total spectral distributions from Hawking radiation
European Physical Journal C: Particles and Fields
author_facet Bogusław Broda
author_sort Bogusław Broda
title Total spectral distributions from Hawking radiation
title_short Total spectral distributions from Hawking radiation
title_full Total spectral distributions from Hawking radiation
title_fullStr Total spectral distributions from Hawking radiation
title_full_unstemmed Total spectral distributions from Hawking radiation
title_sort total spectral distributions from hawking radiation
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2017-11-01
description Abstract Taking into account the time dependence of the Hawking temperature and finite evaporation time of the black hole, the total spectral distributions of the radiant energy and of the number of particles have been explicitly calculated and compared to their temporary (initial) blackbody counterparts (spectral exitances).
url http://link.springer.com/article/10.1140/epjc/s10052-017-5336-1
work_keys_str_mv AT bogusławbroda totalspectraldistributionsfromhawkingradiation
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