Comment on “Quasinormal modes in Schwarzschild–de Sitter spacetime: A simple derivation of the level spacing of the frequencies”

D. Batic, N. G. Kelkar, and M. Nowakowski
Phys. Rev. D 83, 108501 – Published 23 May 2011

Abstract

It is shown here that the extraction of quasinormal modes within the first Born approximation of the scattering amplitude is mathematically not well-founded. Indeed, the constraints on the existence of the scattering amplitude integral lead to inequalities for the imaginary parts of the quasinormal mode frequencies. For instance, in the Schwarzschild case, 0ωI<κ (where κ is the surface gravity at the horizon) invalidates the poles deduced from the first Born approximation method, namely, ωn=inκ.

  • Received 24 November 2010

DOI:https://doi.org/10.1103/PhysRevD.83.108501

© 2011 American Physical Society

Authors & Affiliations

D. Batic1, N. G. Kelkar2, and M. Nowakowski2

  • 1Department of Mathematics, University of the West Indies, Kingston 6, Jamaica
  • 2Departamento de Fisica, Universidad de los Andes, Carrera 1E Numero 18A-10, Bogota, Colombia

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Vol. 83, Iss. 10 — 15 May 2011

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