On the absence of scalar hair for charged rotating blackholes in non minimally coupled theories

Abstract

In this work we check the validity of the no scalar hair theorem in charged axisymmetric stationary black holes for a wide class of scalar tensor theories.

arXiv commentRevtex style, 11 pages, major rivisions done, appendix added, title changed

References in corpus (3)

• A Classical Instability of Reissner-Nordstrom Solutions and the Fate of Magnetically Charged Black Holes
• Black Holes: Classical Properties, Thermodynamics and Heuristic Quantization
• New no-scalar-hair theorem for black-holes

Cited by in corpus (6)

• Spontaneous scalarization
• No hair theorems for stationary axisymmetric black holes
• Note on black hole no hair theorems for massive forms and spin-1/2 fields
• An Exact Interior Kerr Solution
• Massive spin-2 and spin-1/2 no hair theorems for stationary axisymmetric black holes
• On the effect of scalar fields on Hawking radiation and quasinormal modes of black holes