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Electromagnetic quasinormal modes of D-dimensional black holes

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arxiv gr-qc/0605034 v2 pith:UACJJ7FI submitted 2006-05-05 gr-qc

Electromagnetic quasinormal modes of D-dimensional black holes

classification gr-qc
keywords d-dimensionalblackelectromagneticschwarzschildsitteranti-decalculatefrequencies
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Using the monodromy method we calculate the asymptotic quasinormal (QN) frequencies of an electromagnetic field moving in D-dimensional Schwarzschild and Schwarzschild de Sitter (SdS) black holes ($D\geq 4$). For the D-dimensional Schwarzschild anti-de Sitter (SadS) black hole we also compute these frequencies with a similar method. Moreover, we calculate the electromagnetic normal modes of the D-dimensional anti-de Sitter (AdS) spacetime.

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Cited by 4 Pith papers

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

  1. Quasinormal modes of Proca and Maxwell fields in $d$-dimensional Schwarzschild-AdS black holes

    gr-qc 2026-05 conditional novelty 7.0

    Scalar-type Maxwell perturbations in large d≥5 Schwarzschild-AdS black holes exhibit purely imaginary low-frequency quasinormal modes, confirmed numerically and by asymptotic matching.

  2. Grey-body factors of higher dimensional regular black holes in quasi-topological theories

    gr-qc 2026-01 unverdicted novelty 5.0

    Higher dimensional regular black holes in quasi-topological gravity have suppressed grey-body factors and Hawking radiation compared to singular black holes in general relativity.

  3. Grey-body factors of higher dimensional regular black holes in quasi-topological theories

    gr-qc 2026-01 unverdicted novelty 4.0

    Higher-dimensional regular black holes in quasi-topological gravity exhibit significantly suppressed grey-body factors and Hawking evaporation compared to singular black holes in general relativity.

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

    gr-qc 2011-02 accept novelty 1.0

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