Exact black-hole solution with self-interacting scalar field

DOI10.1088/0264-9381/12/6/013zbMath0823.53064arXivgr-qc/9502011OpenAlexW3101490705MaRDI QIDQ4838579

Olaf Bechmann, Olaf Lechtenfeld

Publication date: 12 July 1995

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9502011

zbMATH Keywords

self-interacting scalar fieldblack-hole solutionscalar no-hair theorem

Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (10)

SCALAR DEFORMATIONS OF SCHWARZSCHILD HOLES AND THEIR STABILITY ⋮ On black holes with scalar hairs ⋮ Hairy black holes, scalar charges and extended thermodynamics ⋮ Axially symmetric static scalar solitons and black holes with scalar hair ⋮ Selection criteria for two-parameter solutions to scalar-tensor gravity ⋮ Regular black holes and black universes ⋮ Charged dilaton black holes with unusual asymptotics ⋮ Regular Phantom Black Holes ⋮ A solution-generating method in Einstein-scalar gravity ⋮ Analytic and asymptotically flat hairy (ultra-compact) black-hole solutions and their axial perturbations

This page was built for publication: Exact black-hole solution with self-interacting scalar field