Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler Density
The evaluation of the energy-momentum distribution for a new four-dimensional, spherically symmetric, static and charged black hole spacetime geometry with constant nonzero topological Euler density is performed by using the energy-momentum complexes of Einstein and Møller. This black hole solution...
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| Main Authors: | , , , , , , |
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| Format: | Article |
| Language: | English |
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Wiley
2018-01-01
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| Series: | Advances in High Energy Physics |
| Online Access: | http://dx.doi.org/10.1155/2018/5212696 |
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| author | Irina Radinschi Theophanes Grammenos Farook Rahaman Andromahi Spanou Marius Mihai Cazacu Surajit Chattopadhyay Antonio Pasqua |
| author_facet | Irina Radinschi Theophanes Grammenos Farook Rahaman Andromahi Spanou Marius Mihai Cazacu Surajit Chattopadhyay Antonio Pasqua |
| author_sort | Irina Radinschi |
| collection | DOAJ |
| description | The evaluation of the energy-momentum distribution for a new four-dimensional, spherically symmetric, static and charged black hole spacetime geometry with constant nonzero topological Euler density is performed by using the energy-momentum complexes of Einstein and Møller. This black hole solution was recently developed in the context of the coupled Einstein–nonlinear electrodynamics of the Born-Infeld type. The energy is found to depend on the mass M and the charge q of the black hole, the cosmological constant Λ, and the radial coordinate r, while in both prescriptions all the momenta vanish. Some limiting and particular cases are analyzed and discussed, illustrating the rather extraordinary character of the spacetime geometry considered. |
| format | Article |
| id | doaj-art-919bf65ac7774d7089283dbed9876acc |
| institution | Kabale University |
| issn | 1687-7357 1687-7365 |
| language | English |
| publishDate | 2018-01-01 |
| publisher | Wiley |
| record_format | Article |
| series | Advances in High Energy Physics |
| spelling | doaj-art-919bf65ac7774d7089283dbed9876acc2025-02-03T01:23:29ZengWileyAdvances in High Energy Physics1687-73571687-73652018-01-01201810.1155/2018/52126965212696Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler DensityIrina Radinschi0Theophanes Grammenos1Farook Rahaman2Andromahi Spanou3Marius Mihai Cazacu4Surajit Chattopadhyay5Antonio Pasqua6Department of Physics “Gh. Asachi” Technical University, Iasi 700050, RomaniaDepartment of Civil Engineering, University of Thessaly, 383 34 Volos, GreeceDepartment of Mathematics, Jadavpur University, Kolkata 700 032, West Bengal, IndiaSchool of Applied Mathematics and Physical Sciences, National Technical University of Athens, 157 80 Athens, GreeceDepartment of Physics “Gh. Asachi” Technical University, Iasi 700050, RomaniaDepartment of Mathematics, Amity University, Kolkata 700135, IndiaDepartment of Physics, University of Trieste, 34127 Trieste, ItalyThe evaluation of the energy-momentum distribution for a new four-dimensional, spherically symmetric, static and charged black hole spacetime geometry with constant nonzero topological Euler density is performed by using the energy-momentum complexes of Einstein and Møller. This black hole solution was recently developed in the context of the coupled Einstein–nonlinear electrodynamics of the Born-Infeld type. The energy is found to depend on the mass M and the charge q of the black hole, the cosmological constant Λ, and the radial coordinate r, while in both prescriptions all the momenta vanish. Some limiting and particular cases are analyzed and discussed, illustrating the rather extraordinary character of the spacetime geometry considered.http://dx.doi.org/10.1155/2018/5212696 |
| spellingShingle | Irina Radinschi Theophanes Grammenos Farook Rahaman Andromahi Spanou Marius Mihai Cazacu Surajit Chattopadhyay Antonio Pasqua Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler Density Advances in High Energy Physics |
| title | Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler Density |
| title_full | Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler Density |
| title_fullStr | Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler Density |
| title_full_unstemmed | Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler Density |
| title_short | Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler Density |
| title_sort | localization of energy momentum for a black hole spacetime geometry with constant topological euler density |
| url | http://dx.doi.org/10.1155/2018/5212696 |
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