Remarks on Remnants by Fermions’ Tunnelling from Black Strings

Hawking’s calculation is unable to predict the final stage of the black hole evaporation. When effects of quantum gravity are taken into account, there is a minimal observable length. In this paper, we investigate fermions’ tunnelling from the charged and rotating black strings. With the influence o...

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Main Authors: Deyou Chen, Zhonghua Li
Format: Article
Language:English
Published: Wiley 2014-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2014/620157
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author Deyou Chen
Zhonghua Li
author_facet Deyou Chen
Zhonghua Li
author_sort Deyou Chen
collection DOAJ
description Hawking’s calculation is unable to predict the final stage of the black hole evaporation. When effects of quantum gravity are taken into account, there is a minimal observable length. In this paper, we investigate fermions’ tunnelling from the charged and rotating black strings. With the influence of the generalized uncertainty principle, the Hawking temperatures are not only determined by the rings, but also affected by the quantum numbers of the emitted fermions. Quantum gravity corrections slow down the increases of the temperatures, which naturally leads to remnants left in the evaporation.
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institution Kabale University
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publishDate 2014-01-01
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spelling doaj-art-01e76c95d97342eea4304ab9b876a9462025-02-03T05:45:08ZengWileyAdvances in High Energy Physics1687-73571687-73652014-01-01201410.1155/2014/620157620157Remarks on Remnants by Fermions’ Tunnelling from Black StringsDeyou Chen0Zhonghua Li1Institute of Theoretical Physics, China West Normal University, Nanchong 637009, ChinaInstitute of Theoretical Physics, China West Normal University, Nanchong 637009, ChinaHawking’s calculation is unable to predict the final stage of the black hole evaporation. When effects of quantum gravity are taken into account, there is a minimal observable length. In this paper, we investigate fermions’ tunnelling from the charged and rotating black strings. With the influence of the generalized uncertainty principle, the Hawking temperatures are not only determined by the rings, but also affected by the quantum numbers of the emitted fermions. Quantum gravity corrections slow down the increases of the temperatures, which naturally leads to remnants left in the evaporation.http://dx.doi.org/10.1155/2014/620157
spellingShingle Deyou Chen
Zhonghua Li
Remarks on Remnants by Fermions’ Tunnelling from Black Strings
Advances in High Energy Physics
title Remarks on Remnants by Fermions’ Tunnelling from Black Strings
title_full Remarks on Remnants by Fermions’ Tunnelling from Black Strings
title_fullStr Remarks on Remnants by Fermions’ Tunnelling from Black Strings
title_full_unstemmed Remarks on Remnants by Fermions’ Tunnelling from Black Strings
title_short Remarks on Remnants by Fermions’ Tunnelling from Black Strings
title_sort remarks on remnants by fermions tunnelling from black strings
url http://dx.doi.org/10.1155/2014/620157
work_keys_str_mv AT deyouchen remarksonremnantsbyfermionstunnellingfromblackstrings
AT zhonghuali remarksonremnantsbyfermionstunnellingfromblackstrings