Stationary BTZ space-time in Ricci-inverse and $$f({\mathcal {R}})$$ f ( R ) gravity theories
Abstract In this paper, we explore a stationary BTZ space-time within the framework of modified gravity theory, specifically focusing on Ricci-inverse gravity. It is important to clarify that “Ricci-inverse” refers to the inverse of the Ricci tensor, not the Ricci scalar. We consider a general class...
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SpringerOpen
2024-12-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | https://doi.org/10.1140/epjc/s10052-024-13637-1 |
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| author | Faizuddin Ahmed Abdelmalek Bouzenada |
| author_facet | Faizuddin Ahmed Abdelmalek Bouzenada |
| author_sort | Faizuddin Ahmed |
| collection | DOAJ |
| description | Abstract In this paper, we explore a stationary BTZ space-time within the framework of modified gravity theory, specifically focusing on Ricci-inverse gravity. It is important to clarify that “Ricci-inverse” refers to the inverse of the Ricci tensor, not the Ricci scalar. We consider a general class of this gravity theory, where the function f is defined by $$f({\mathcal {R}}, {\mathcal {A}}, A^{\mu \nu }\,A_{\mu \nu })$$ f ( R , A , A μ ν A μ ν ) , with $${\mathcal {R}}$$ R and $${\mathcal {A}}$$ A representing the Ricci and anti-curvature scalars, respectively and $$A^{\mu \nu }$$ A μ ν is the anti-curvature tensor. We demonstrate that stationary BTZ space-time is a valid solution in this gravity theory, wherein the cosmological constant undergoes modifications due to the coupling constants. Moreover, we study another modified gravity theory known as $$f({\mathcal {R}})$$ f ( R ) -gravity and analyze the stationary BTZ space-time. Subsequently, we fully integrate the geodesic equations for BTZ space-time constructed within the Ricci-Inverse gravity, expressing the solutions in terms of elementary functions and compared with the GR result. We classify different types of geodesics, including null and time-like geodesics, under three conditions: (i) nonzero mass and angular momentum, $$M \ne 0, J\ne 0$$ M ≠ 0 , J ≠ 0 , (ii) massless BTZ space-time, $$M=0$$ M = 0 and $$J=0$$ J = 0 , and (iii) $$M=-1, J=0$$ M = - 1 , J = 0 , that is $$AdS_3$$ A d S 3 -type, and analyze the results in modified gravity theories and compare with the general relativity case. |
| format | Article |
| id | doaj-art-d5b1263de34e460f8136f2fb3e5aad54 |
| institution | Kabale University |
| issn | 1434-6052 |
| language | English |
| publishDate | 2024-12-01 |
| publisher | SpringerOpen |
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| series | European Physical Journal C: Particles and Fields |
| spelling | doaj-art-d5b1263de34e460f8136f2fb3e5aad542025-02-02T12:39:24ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522024-12-01841211610.1140/epjc/s10052-024-13637-1Stationary BTZ space-time in Ricci-inverse and $$f({\mathcal {R}})$$ f ( R ) gravity theoriesFaizuddin Ahmed0Abdelmalek Bouzenada1Department of Physics, University of Science and Technology MeghalayaLaboratory of Theoretical and Applied Physics, Echahid Cheikh Larbi Tebessi UniversityAbstract In this paper, we explore a stationary BTZ space-time within the framework of modified gravity theory, specifically focusing on Ricci-inverse gravity. It is important to clarify that “Ricci-inverse” refers to the inverse of the Ricci tensor, not the Ricci scalar. We consider a general class of this gravity theory, where the function f is defined by $$f({\mathcal {R}}, {\mathcal {A}}, A^{\mu \nu }\,A_{\mu \nu })$$ f ( R , A , A μ ν A μ ν ) , with $${\mathcal {R}}$$ R and $${\mathcal {A}}$$ A representing the Ricci and anti-curvature scalars, respectively and $$A^{\mu \nu }$$ A μ ν is the anti-curvature tensor. We demonstrate that stationary BTZ space-time is a valid solution in this gravity theory, wherein the cosmological constant undergoes modifications due to the coupling constants. Moreover, we study another modified gravity theory known as $$f({\mathcal {R}})$$ f ( R ) -gravity and analyze the stationary BTZ space-time. Subsequently, we fully integrate the geodesic equations for BTZ space-time constructed within the Ricci-Inverse gravity, expressing the solutions in terms of elementary functions and compared with the GR result. We classify different types of geodesics, including null and time-like geodesics, under three conditions: (i) nonzero mass and angular momentum, $$M \ne 0, J\ne 0$$ M ≠ 0 , J ≠ 0 , (ii) massless BTZ space-time, $$M=0$$ M = 0 and $$J=0$$ J = 0 , and (iii) $$M=-1, J=0$$ M = - 1 , J = 0 , that is $$AdS_3$$ A d S 3 -type, and analyze the results in modified gravity theories and compare with the general relativity case.https://doi.org/10.1140/epjc/s10052-024-13637-1 |
| spellingShingle | Faizuddin Ahmed Abdelmalek Bouzenada Stationary BTZ space-time in Ricci-inverse and $$f({\mathcal {R}})$$ f ( R ) gravity theories European Physical Journal C: Particles and Fields |
| title | Stationary BTZ space-time in Ricci-inverse and $$f({\mathcal {R}})$$ f ( R ) gravity theories |
| title_full | Stationary BTZ space-time in Ricci-inverse and $$f({\mathcal {R}})$$ f ( R ) gravity theories |
| title_fullStr | Stationary BTZ space-time in Ricci-inverse and $$f({\mathcal {R}})$$ f ( R ) gravity theories |
| title_full_unstemmed | Stationary BTZ space-time in Ricci-inverse and $$f({\mathcal {R}})$$ f ( R ) gravity theories |
| title_short | Stationary BTZ space-time in Ricci-inverse and $$f({\mathcal {R}})$$ f ( R ) gravity theories |
| title_sort | stationary btz space time in ricci inverse and f mathcal r f r gravity theories |
| url | https://doi.org/10.1140/epjc/s10052-024-13637-1 |
| work_keys_str_mv | AT faizuddinahmed stationarybtzspacetimeinricciinverseandfmathcalrfrgravitytheories AT abdelmalekbouzenada stationarybtzspacetimeinricciinverseandfmathcalrfrgravitytheories |