Dynamics of charged and rotating NUT black holes in Rastall gravity

DOI10.1142/S0218271820500212zbMath1434.83073arXiv1908.09629OpenAlexW3102349640WikidataQ126396896 ScholiaQ126396896MaRDI QIDQ5109436

Getbogi Hikmawan, Freddy P. Zen, M. F. A. R. Sakti, Unnamed Author

Publication date: 12 May 2020

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1908.09629

zbMATH Keywords

thermodynamicsblack holeevent horizonRastall gravityequatorial circular orbit

Mathematics Subject Classification ID

Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (6)

Effects of Rastall parameter on perturbation of dark sectors of the Universe ⋮ Isotropic compact stellar model in Rastall's gravitational theory ⋮ Fermionic and bosonic greybody factors as well as quasinormal modes for charged Taub NUT black holes ⋮ Kerr-Newman-NUT-Kiselev black holes in Rastall theory of gravity and Kerr/CFT correspondence ⋮ On black holes surrounded by a fluid of strings in Rastall gravity ⋮ Observable characteristics of the charged black hole surrounded by thin disk accretion in Rastall gravity

Cites Work

• On the physical meaning of the NUT parameter
• Center of mass energy of the collision for two general geodesic particles around a Kerr-Newman-Taub-NUT black hole
• Generalization of the Einstein Theory
• Classical monopoles: Newton, NUT space, gravomagnetic lensing, and atomic spectra
• DYNAMICS OF DARK ENERGY
• Circular geodesics in the Kerr–Newman–Taub–NUT spacetime
• Quintessence and black holes
• Empty-Space Generalization of the Schwarzschild Metric
• Empty space-times admitting a three parameter group of motions

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