Quasinormal modes of stringy black holes

Details Quasinormal modes of stringy black holes Quasinormal modes of stringy black holes

2002-05-02

arxiv.org/abs/gr-qc/0205007v1

Phys.Lett. B507 (2001) 312-316

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

2 figures

Scientific paper

10.1016/S0370-2693(01)00437-3

String theory is a promising candidate for a fundamental quantum theory of all interactions including Einstein gravity. Some solutions in string theory can be interpreted as black holes. Using the semi-analytic method and WKB method,the quasinormal modes(QNMs)of 1+1 dimensional black hole in string theory are studied.The QNMs of 1+3 dimensional black hole in string theory are also calculated through numerical approach.The numerical investigation has shown that the late time gravitational oscillation of the black hole under an external perturbaton is dominated by certain QNMs.

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