Quasi-normal modes, bifurcations and non-uniqueness of charged scalar-tensor black holes

Details Quasi-normal modes, bifurcations and non-uniqueness of charged scalar-tensor black holes Quasi-normal modes, bifurcations and non-uniqueness of charged scalar-tensor black holes

2010-07-11

arxiv.org/abs/1007.1767v2

Phys.Rev.D82:064030,2010

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

22 pages, 11 figures; v2: typos corrected, comments and references added

Scientific paper

10.1103/PhysRevD.82.064030

In the present paper we study the scalar sector of the quasinormal modes of charged general relativistic, static and spherically symmetric black holes coupled to nonlinear electrodynamics and embedded in a class of scalar-tensor theories. We find that for certain domain of the parametric space there exist unstable quasinormal modes. The presence of instabilities implies the existence of scalar-tensor black holes with primary hair that bifurcate from the embedded general relativistic black-hole solutions at critical values of the parameters corresponding to the static zero-modes. We prove that such scalar-tensor black holes really exist by solving the full system of scalar-tensor field equations for the static, spherically symmetric case. The obtained solutions for the hairy black holes are non-unique and they are in one to one correspondence with the bounded states of the potential governing the linear perturbations of the scalar field. The stability of the non-unique hairy black holes is also examined and we find that the solutions for which the scalar field has zeros are unstable against radial perturbations. The paper ends with a discussion on possible formulations of a new classification conjecture.

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