A class of black holes in dRGT massive gravity and their thermodynamical properties
© 2016, The Author(s). We present an exact spherical black hole solution in de Rham, Gabadadze, and Tolley (dRGT) massive gravity for a generic choice of the parameters in the theory, and also discuss the thermodynamical and phase structure of the black hole in both the grand canonical and the canon...
Saved in:
Main Authors: | , , |
---|---|
Other Authors: | |
Format: | Article |
Published: |
2018
|
Subjects: | |
Online Access: | https://repository.li.mahidol.ac.th/handle/123456789/40592 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Institution: | Mahidol University |
id |
th-mahidol.40592 |
---|---|
record_format |
dspace |
spelling |
th-mahidol.405922019-03-14T15:01:27Z A class of black holes in dRGT massive gravity and their thermodynamical properties Suchant G. Ghosh Lunchakorn Tannukij Pitayuth Wongjun Jamia Millia Islamia University of KwaZulu-Natal Mahidol University Naresuan University Thailand Ministry of Education Engineering © 2016, The Author(s). We present an exact spherical black hole solution in de Rham, Gabadadze, and Tolley (dRGT) massive gravity for a generic choice of the parameters in the theory, and also discuss the thermodynamical and phase structure of the black hole in both the grand canonical and the canonical ensembles (for the charged case). It turns out that the dRGT black hole solution includes other known solutions to the Einstein field equations, such as the monopole-de Sitter–Schwarzschild solution with the coefficients of the third and fourth terms in the potential and the graviton mass in massive gravity naturally generates the cosmological constant and the global monopole term. Furthermore, we compute the mass, temperature and entropy of the dRGT black hole, and also perform thermodynamical stability analysis. It turns out that the presence of the graviton mass completely changes the black hole thermodynamics, and it can provide the Hawking–Page phase transition which also occurs for the charged black holes. Interestingly, the entropy of a black hole is barely affected and still obeys the standard area law. In particular, our results, in the limit (Formula presented.) , reduced exactly to the results of general relativity. 2018-12-11T02:49:04Z 2019-03-14T08:01:27Z 2018-12-11T02:49:04Z 2019-03-14T08:01:27Z 2016-03-01 Article European Physical Journal C. Vol.76, No.3 (2016) 10.1140/epjc/s10052-016-3943-x 14346052 14346044 2-s2.0-84959546487 https://repository.li.mahidol.ac.th/handle/123456789/40592 Mahidol University SCOPUS https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84959546487&origin=inward |
institution |
Mahidol University |
building |
Mahidol University Library |
continent |
Asia |
country |
Thailand Thailand |
content_provider |
Mahidol University Library |
collection |
Mahidol University Institutional Repository |
topic |
Engineering |
spellingShingle |
Engineering Suchant G. Ghosh Lunchakorn Tannukij Pitayuth Wongjun A class of black holes in dRGT massive gravity and their thermodynamical properties |
description |
© 2016, The Author(s). We present an exact spherical black hole solution in de Rham, Gabadadze, and Tolley (dRGT) massive gravity for a generic choice of the parameters in the theory, and also discuss the thermodynamical and phase structure of the black hole in both the grand canonical and the canonical ensembles (for the charged case). It turns out that the dRGT black hole solution includes other known solutions to the Einstein field equations, such as the monopole-de Sitter–Schwarzschild solution with the coefficients of the third and fourth terms in the potential and the graviton mass in massive gravity naturally generates the cosmological constant and the global monopole term. Furthermore, we compute the mass, temperature and entropy of the dRGT black hole, and also perform thermodynamical stability analysis. It turns out that the presence of the graviton mass completely changes the black hole thermodynamics, and it can provide the Hawking–Page phase transition which also occurs for the charged black holes. Interestingly, the entropy of a black hole is barely affected and still obeys the standard area law. In particular, our results, in the limit (Formula presented.) , reduced exactly to the results of general relativity. |
author2 |
Jamia Millia Islamia |
author_facet |
Jamia Millia Islamia Suchant G. Ghosh Lunchakorn Tannukij Pitayuth Wongjun |
format |
Article |
author |
Suchant G. Ghosh Lunchakorn Tannukij Pitayuth Wongjun |
author_sort |
Suchant G. Ghosh |
title |
A class of black holes in dRGT massive gravity and their thermodynamical properties |
title_short |
A class of black holes in dRGT massive gravity and their thermodynamical properties |
title_full |
A class of black holes in dRGT massive gravity and their thermodynamical properties |
title_fullStr |
A class of black holes in dRGT massive gravity and their thermodynamical properties |
title_full_unstemmed |
A class of black holes in dRGT massive gravity and their thermodynamical properties |
title_sort |
class of black holes in drgt massive gravity and their thermodynamical properties |
publishDate |
2018 |
url |
https://repository.li.mahidol.ac.th/handle/123456789/40592 |
_version_ |
1763491703195435008 |