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    Quasinormal modes for the Vaidya metric

    Elcio Abdalla* and Cecilia B. M. H. Chirenti†

    Alberto Saa‡

    • Instituto de Física, Universidade de São Paulo, C.P. 66318, 05315-970—São Paulo, SP, Brazil

    • Departamento de Matemática Aplicada, UNICAMP, C.P. 6065, 13083-859—Campinas, SP, Brazil

    • *Electronic address: eabdalla@fma.if.usp.br
    • †Electronic address: cecilia@fma.if.usp.br
    • ‡Electronic address: asaa@ime.unicamp.br

    Phys. Rev. D 74, 084029 – Published 25 October, 2006

    DOI: https://doi.org/10.1103/PhysRevD.74.084029

    Abstract

    We consider here scalar and electromagnetic perturbations for the Vaidya metric in double-null coordinates. Such an approach allows one to go a step further in the analysis of quasinormal modes for time-dependent spacetimes. Some recent results are refined, and a new nonstationary behavior corresponding to some sort of inertia for quasinormal modes is identified. Our conclusions can enlighten some aspects of the wave scattering by black holes undergoing some mass accretion processes.

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