Phenomenological Extension for Tidal Charge Black Hole
A simple phenomenological extension of the black hole solution with tidal charge is proposed. Empirical data on the Sgr A* black hole is consistent with the suggested metric which serves as a generalization of the Reissner–Nordström one. Such a generalization includes the leading effects beyond gene...
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| Veröffentlicht in: | Journal of experimental and theoretical physics 2019-05, Vol.128 (5), p.720-726 |
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| container_issue | 5 |
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| container_title | Journal of experimental and theoretical physics |
| container_volume | 128 |
| creator | Alexeyev, S. O. Latosh, B. N. Prokopov, V. A. Emtsova, E. D. |
| description | A simple phenomenological extension of the black hole solution with tidal charge is proposed. Empirical data on the Sgr A* black hole is consistent with the suggested metric which serves as a generalization of the Reissner–Nordström one. Such a generalization includes the leading effects beyond general relativity; so, the discussed metric can explain wider range of gravitational effects. We discuss physical features of an object described by the proposed metric, namely, the size of its shadow and the innermost stable circular orbit radius. |
| doi_str_mv | 10.1134/S1063776119040010 |
| format | Article |
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| subjects | Astronomy Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BLACK HOLES Circular orbits Classical and Quantum Gravitation Elementary Particles Fields GENERAL RELATIVITY THEORY GRAVITATION Gravitational effects METRICS Nuclei Orbital stability Orbits (Astrophysics) Particle and Nuclear Physics Particles Physics Physics and Astronomy Quantum Field Theory Quantum mechanics Relativity Relativity Theory Solid State Physics Universities and colleges |
| title | Phenomenological Extension for Tidal Charge Black Hole |
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