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Quasinormal modes of stringy black holes

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arxiv gr-qc/0205007 v1 pith:RFIDQXF3 submitted 2002-05-02 gr-qc

Xin-zhou Li , Jian-gang Hao , Dao-jun Liu This is my paper
classification gr-qc
keywords blacktheorystringholeqnmsdimensionalholesmethod
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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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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. New analytic solutions of non-SUSY black branes in $10$-D heterotic supergravity and the phase transition

    hep-th 2025-12 unverdicted novelty 5.0 of 10

    New exact non-SUSY black brane solutions in 10D heterotic supergravity with two gauge charges show a spontaneous symmetry breaking and dynamical instability at low temperature that predicts additional black hole solutions.

  2. Quasinormal modes of black holes: from astrophysics to string theory

    gr-qc 2011-02 accept novelty 1.0 of 10

    This review surveys calculations and interpretations of quasinormal modes for black holes in astrophysics, higher dimensions, and holographic duals without presenting new results.

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