SCALAR DEFORMATIONS OF SCHWARZSCHILD HOLES AND THEIR STABILITY

DOI10.1142/S0217751X98000329zbMath0921.53048arXivgr-qc/9612062MaRDI QIDQ4259585

Helge Dennhardt, Olaf Lechtenfeld

Publication date: 2 September 1999

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

Full work available at URL: https://arxiv.org/abs/gr-qc/9612062

zbMATH Keywords

no-hair theoremlinear perturbation theorydeformations of Schwarzschild black holesminimally coupled Einstein-scalar field equations

Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05)

Related Items (11)

On black holes with scalar hairs ⋮ Hairy black holes, scalar charges and extended thermodynamics ⋮ Linear stability of Mandal–Sengupta–Wadia black holes ⋮ Effective field theory of black hole quasinormal modes in scalar-tensor theories ⋮ Axially symmetric static scalar solitons and black holes with scalar hair ⋮ No inner-horizon theorem for black holes with charged scalar hairs ⋮ Spherically symmetric gravitating scalar field. The inverse problem and exact solutions ⋮ Regular Phantom Black Holes ⋮ A solution-generating method in Einstein-scalar gravity ⋮ Effective field theory for the perturbations of a slowly rotating black hole ⋮ Analytic and asymptotically flat hairy (ultra-compact) black-hole solutions and their axial perturbations

Cites Work

• Stability of a Schwarzschild Singularity
• Reciprocal Static Metrics and Scalar Fields in the General Theory of Relativity
• Exact black-hole solution with self-interacting scalar field

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