Black hole solutions in Rastall theory

2016/10/31 by Y. Heydarzade, H. Moradpour, F. Darabi · 3 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Noncommutative and Quantum Gravity Theories

paper · doi:10.1139/cjp-2017-0254

openalex created_date 2016/10/28 · openalex publication_date 2017/06/02 · crossref created 2017/06/02 · crossref issued 2017/12/01 · crossref published 2017/12/01 · crossref published-print 2017/12/01 · crossref deposited 2025/07/02 · crossref indexed 2026/07/29 · openalex updated_date 2026/07/29

Abstract

The Reissner–Nordström black hole solution in a generic cosmological constant background in the context of Rastall gravity is obtained. It is shown that the cosmological constant arises naturally from the consistency of the non-vacuum field equations of the Rastall theory for a spherical symmetric space–time, rather than its ad hoc introduction in the usual Einstein and Einstein–Maxwell field equations. The usual Reissner–Nordström, Schwarzschild, and Schwarzschild – (anti-)de Sitter black hole solutions in the framework of this theory are also addressed as the special independent subclasses of the obtained general solution.

Citations

• Quantum Fields in Curved Space
• Observation of Gravitational Waves from a Binary Black Hole Merger

Cited by

• The sound of quintessence: analogue Kiselev acoustic black holes
• Non-commutative wormholes exhibiting conformal motion in Rastall gravity
• Maximum mass of singularity-free anisotropic compact stars in Rastall theory of gravity
• Einstein Maxwell Scalar Black Hole: Thermodynamic Properties with Logarithmic Barrow Entropy

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