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, ${\ensuremath{\omega}}_{n}=in\ensuremath{\kappa}$.

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.