A no-hair theorem for spherically symmetric black holes in \(R^2\) gravity

DOI10.1007/S10714-018-2463-4zbMath1403.83044arXiv1810.02915OpenAlexW2895566185MaRDI QIDQ1618036

Demosthenes Kazanas, Joseph Sultana

Publication date: 13 November 2018

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1810.02915

zbMATH Keywords

black holesscalar fieldno-hair theorems\(R^2\) gravityHiggs-type quartic potentialscalar tensor representation of general \(f(R)\) theory

Mathematics Subject Classification ID

Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (7)

On instabilities of stationary scalar field configurations supported by reflecting compact stars ⋮ Test of conformal theory of gravity as an alternative paradigm to dark matter hypothesis from gravitational lensing studies ⋮ Spherical inhomogeneous solutions of Einstein and scalar-tensor gravity: a map of the land ⋮ Analytic charged BHs in \(f(R)\) gravity ⋮ Gravitational analog of the canonical acoustic black hole in Einstein–scalar–Gauss–Bonnet theory ⋮ Null trajectories and bending of light in charged black holes with quintessence ⋮ Neutron stars inf(R) gravity and scalar-tensor theories

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