Rotating black hole in Rastall theory
Rotating black hole solutions in theories of modified gravity are important as they offer an arena to test these theories through astrophysical observation. The non-rotating black hole can be hardly tested since the black hole spin is very important in any astrophysical process. We present rotating...
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| Published in | The European physical journal. C, Particles and fields Vol. 78; no. 9; pp. 1 - 13 |
|---|---|
| Main Authors | , |
| Format | Journal Article |
| Language | English |
| Published |
Berlin/Heidelberg
Springer Berlin Heidelberg
01.09.2018
Springer Springer Nature B.V SpringerOpen |
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| Online Access | Get full text |
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| Abstract | Rotating black hole solutions in theories of modified gravity are important as they offer an arena to test these theories through astrophysical observation. The non-rotating black hole can be hardly tested since the black hole spin is very important in any astrophysical process. We present rotating counterpart of a recently obtained spherically symmetric exact black hole solution surrounded by perfect fluid in the context of Rastall theory, viz, rotating Rastall black hole that generalize the Kerr–Newman black hole solution. In turn, we analyze the specific cases of the Kerr–Newman black holes surrounded by matter like dust and quintessence fields. Interestingly, for a set of parameters and a chosen surrounding field, there exists a critical rotation parameter (
a
=
a
E
), which corresponds to an extremal black hole with degenerate horizons, while for
a
<
a
E
, it describes a non-extremal black hole with Cauchy and event horizons, and no black hole for
a
>
a
E
with value
a
E
is also influenced by these parameters. We also discuss the thermodynamical quantities associated with rotating Rastall black hole, and analyze the particle motion with the behavior of effective potential. |
|---|---|
| AbstractList | Abstract Rotating black hole solutions in theories of modified gravity are important as they offer an arena to test these theories through astrophysical observation. The non-rotating black hole can be hardly tested since the black hole spin is very important in any astrophysical process. We present rotating counterpart of a recently obtained spherically symmetric exact black hole solution surrounded by perfect fluid in the context of Rastall theory, viz, rotating Rastall black hole that generalize the Kerr–Newman black hole solution. In turn, we analyze the specific cases of the Kerr–Newman black holes surrounded by matter like dust and quintessence fields. Interestingly, for a set of parameters and a chosen surrounding field, there exists a critical rotation parameter ($$a=a_{E}$$ a=aE ), which corresponds to an extremal black hole with degenerate horizons, while for $$a<a_{E}$$ a<aE , it describes a non-extremal black hole with Cauchy and event horizons, and no black hole for $$a>a_{E}$$ a>aE with value $$a_E$$ aE is also influenced by these parameters. We also discuss the thermodynamical quantities associated with rotating Rastall black hole, and analyze the particle motion with the behavior of effective potential. Rotating black hole solutions in theories of modified gravity are important as they offer an arena to test these theories through astrophysical observation. The non-rotating black hole can be hardly tested since the black hole spin is very important in any astrophysical process. We present rotating counterpart of a recently obtained spherically symmetric exact black hole solution surrounded by perfect fluid in the context of Rastall theory, viz, rotating Rastall black hole that generalize the Kerr–Newman black hole solution. In turn, we analyze the specific cases of the Kerr–Newman black holes surrounded by matter like dust and quintessence fields. Interestingly, for a set of parameters and a chosen surrounding field, there exists a critical rotation parameter (\[a=a_{E}\]), which corresponds to an extremal black hole with degenerate horizons, while for \[a<a_{E}\], it describes a non-extremal black hole with Cauchy and event horizons, and no black hole for \[a>a_{E}\] with value \[a_E\] is also influenced by these parameters. We also discuss the thermodynamical quantities associated with rotating Rastall black hole, and analyze the particle motion with the behavior of effective potential. Rotating black hole solutions in theories of modified gravity are important as they offer an arena to test these theories through astrophysical observation. The non-rotating black hole can be hardly tested since the black hole spin is very important in any astrophysical process. We present rotating counterpart of a recently obtained spherically symmetric exact black hole solution surrounded by perfect fluid in the context of Rastall theory, viz, rotating Rastall black hole that generalize the Kerr-Newman black hole solution. In turn, we analyze the specific cases of the Kerr-Newman black holes surrounded by matter like dust and quintessence fields. Interestingly, for a set of parameters and a chosen surrounding field, there exists a critical rotation parameter ( [Formula omitted]), which corresponds to an extremal black hole with degenerate horizons, while for [Formula omitted], it describes a non-extremal black hole with Cauchy and event horizons, and no black hole for [Formula omitted] with value [Formula omitted] is also influenced by these parameters. We also discuss the thermodynamical quantities associated with rotating Rastall black hole, and analyze the particle motion with the behavior of effective potential. Rotating black hole solutions in theories of modified gravity are important as they offer an arena to test these theories through astrophysical observation. The non-rotating black hole can be hardly tested since the black hole spin is very important in any astrophysical process. We present rotating counterpart of a recently obtained spherically symmetric exact black hole solution surrounded by perfect fluid in the context of Rastall theory, viz, rotating Rastall black hole that generalize the Kerr–Newman black hole solution. In turn, we analyze the specific cases of the Kerr–Newman black holes surrounded by matter like dust and quintessence fields. Interestingly, for a set of parameters and a chosen surrounding field, there exists a critical rotation parameter ( a = a E ), which corresponds to an extremal black hole with degenerate horizons, while for a < a E , it describes a non-extremal black hole with Cauchy and event horizons, and no black hole for a > a E with value a E is also influenced by these parameters. We also discuss the thermodynamical quantities associated with rotating Rastall black hole, and analyze the particle motion with the behavior of effective potential. |
| ArticleNumber | 750 |
| Audience | Academic |
| Author | Kumar, Rahul Ghosh, Sushant G. |
| Author_xml | – sequence: 1 givenname: Rahul surname: Kumar fullname: Kumar, Rahul email: rahul.phy3@gmail.com organization: Centre for Theoretical Physics, Jamia Millia Islamia – sequence: 2 givenname: Sushant G. surname: Ghosh fullname: Ghosh, Sushant G. organization: Centre for Theoretical Physics, Jamia Millia Islamia, Multidisciplinary Centre for Advanced Research and Studies (MCARS), Jamia Millia Islamia, Astrophysics and Cosmology Research Unit, School of Mathematics, Statistics and Computer Science, University of KwaZulu-Natal |
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| Snippet | Rotating black hole solutions in theories of modified gravity are important as they offer an arena to test these theories through astrophysical observation.... Abstract Rotating black hole solutions in theories of modified gravity are important as they offer an arena to test these theories through astrophysical... |
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| SubjectTerms | Astronomy Astrophysics and Cosmology Black holes Elementary Particles Hadrons Heavy Ions Measurement Science and Instrumentation Nuclear Energy Nuclear Physics Parameters Particle motion Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Regular Article - Theoretical Physics Rotation String Theory |
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| Title | Rotating black hole in Rastall theory |
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