An application of Lorentz-invariance violation in black hole thermodynamics

Abstract In this paper, we have applied the Lorentz-invariance violation (LIV) class of dispersion relations (DRs) with the dimensionless parameter $$\textit{n}=2$$ n=2 and the “sign of LIV” $$\eta _+ = 1$$ η+=1 , to a phenomenological study of the effect of quantum gravity in a strong gravitational...

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Main Authors: Guo-Ping Li, Jin Pu, Qing-Quan Jiang, Xiao-Tao Zu
Format: Article
Language:English
Published: SpringerOpen 2017-10-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-017-5220-z
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spelling doaj-472223738aca47fd947fc6c5c97d8ff62020-11-25T00:33:51ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522017-10-01771011010.1140/epjc/s10052-017-5220-zAn application of Lorentz-invariance violation in black hole thermodynamicsGuo-Ping Li0Jin Pu1Qing-Quan Jiang2Xiao-Tao Zu3School of Physical Electronics, University of Electronic Science and Technology of ChinaSchool of Physical Electronics, University of Electronic Science and Technology of ChinaCollege of Physics and Space Science, China West Normal UniversitySchool of Physical Electronics, University of Electronic Science and Technology of ChinaAbstract In this paper, we have applied the Lorentz-invariance violation (LIV) class of dispersion relations (DRs) with the dimensionless parameter $$\textit{n}=2$$ n=2 and the “sign of LIV” $$\eta _+ = 1$$ η+=1 , to a phenomenological study of the effect of quantum gravity in a strong gravitational field. Specifically, we have studied the effect of the LIV-DR induced quantum gravity on the Schwarzschild black hole thermodynamics. The result shows that the effect of the LIV-DR induced quantum gravity speeds up the black hole evaporation, and its corresponding black hole entropy undergoes a leading logarithmic correction to the “reduced Bekenstein–Hawking entropy”, and the ill-defined situations (i.e. the singularity problem and the critical problem) are naturally bypassed when the LIV-DR effect is present. Also, to put our results in a proper perspective, we have compared results with the earlier findings by another quantum-gravity candidate, i.e. the generalized uncertainty principle (GUP). Finally, we conclude from the inert remnants at the final stage of the black hole evaporation that, the GUP as a candidate for describing quantum gravity can always do as well as the LIV-DR by adjusting the model-dependent parameters, but in the same model-dependent parameters the LIV-DR acts as a more suitable candidate.http://link.springer.com/article/10.1140/epjc/s10052-017-5220-z
collection DOAJ
language English
format Article
sources DOAJ
author Guo-Ping Li
Jin Pu
Qing-Quan Jiang
Xiao-Tao Zu
spellingShingle Guo-Ping Li
Jin Pu
Qing-Quan Jiang
Xiao-Tao Zu
An application of Lorentz-invariance violation in black hole thermodynamics
European Physical Journal C: Particles and Fields
author_facet Guo-Ping Li
Jin Pu
Qing-Quan Jiang
Xiao-Tao Zu
author_sort Guo-Ping Li
title An application of Lorentz-invariance violation in black hole thermodynamics
title_short An application of Lorentz-invariance violation in black hole thermodynamics
title_full An application of Lorentz-invariance violation in black hole thermodynamics
title_fullStr An application of Lorentz-invariance violation in black hole thermodynamics
title_full_unstemmed An application of Lorentz-invariance violation in black hole thermodynamics
title_sort application of lorentz-invariance violation in black hole thermodynamics
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2017-10-01
description Abstract In this paper, we have applied the Lorentz-invariance violation (LIV) class of dispersion relations (DRs) with the dimensionless parameter $$\textit{n}=2$$ n=2 and the “sign of LIV” $$\eta _+ = 1$$ η+=1 , to a phenomenological study of the effect of quantum gravity in a strong gravitational field. Specifically, we have studied the effect of the LIV-DR induced quantum gravity on the Schwarzschild black hole thermodynamics. The result shows that the effect of the LIV-DR induced quantum gravity speeds up the black hole evaporation, and its corresponding black hole entropy undergoes a leading logarithmic correction to the “reduced Bekenstein–Hawking entropy”, and the ill-defined situations (i.e. the singularity problem and the critical problem) are naturally bypassed when the LIV-DR effect is present. Also, to put our results in a proper perspective, we have compared results with the earlier findings by another quantum-gravity candidate, i.e. the generalized uncertainty principle (GUP). Finally, we conclude from the inert remnants at the final stage of the black hole evaporation that, the GUP as a candidate for describing quantum gravity can always do as well as the LIV-DR by adjusting the model-dependent parameters, but in the same model-dependent parameters the LIV-DR acts as a more suitable candidate.
url http://link.springer.com/article/10.1140/epjc/s10052-017-5220-z
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