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, $0\ensuremath{\le}{\ensuremath{\omega}}_{I}<\ensuremath{\kappa}$ (where $\ensuremath{\kappa}$ is the surface gravity at the horizon) invalidates the poles deduced from the first Born approximation method, namely, ${\ensuremath{\omega}}_{n}=in\ensuremath{\kappa}$.

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