Rotating black hole in Rastall theory
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...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
SpringerOpen
2018-09-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | http://link.springer.com/article/10.1140/epjc/s10052-018-6206-1 |
| _version_ | 1818491581538238464 |
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| author | Rahul Kumar Sushant G. Ghosh |
| author_facet | Rahul Kumar Sushant G. Ghosh |
| author_sort | Rahul Kumar |
| collection | DOAJ |
| description | 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. |
| first_indexed | 2024-12-10T17:32:55Z |
| format | Article |
| id | doaj.art-9cc4cd65ebb2464fa9f1acc674bfdb56 |
| institution | Directory Open Access Journal |
| issn | 1434-6044 1434-6052 |
| language | English |
| last_indexed | 2024-12-10T17:32:55Z |
| publishDate | 2018-09-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | European Physical Journal C: Particles and Fields |
| spelling | doaj.art-9cc4cd65ebb2464fa9f1acc674bfdb562022-12-22T01:39:37ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-09-0178911310.1140/epjc/s10052-018-6206-1Rotating black hole in Rastall theoryRahul Kumar0Sushant G. Ghosh1Centre for Theoretical Physics, Jamia Millia IslamiaCentre for Theoretical Physics, Jamia Millia IslamiaAbstract 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.http://link.springer.com/article/10.1140/epjc/s10052-018-6206-1 |
| spellingShingle | Rahul Kumar Sushant G. Ghosh Rotating black hole in Rastall theory European Physical Journal C: Particles and Fields |
| title | Rotating black hole in Rastall theory |
| title_full | Rotating black hole in Rastall theory |
| title_fullStr | Rotating black hole in Rastall theory |
| title_full_unstemmed | Rotating black hole in Rastall theory |
| title_short | Rotating black hole in Rastall theory |
| title_sort | rotating black hole in rastall theory |
| url | http://link.springer.com/article/10.1140/epjc/s10052-018-6206-1 |
| work_keys_str_mv | AT rahulkumar rotatingblackholeinrastalltheory AT sushantgghosh rotatingblackholeinrastalltheory |