Abstract
What should be the quasinormal modes associated with a spacetime that contains a naked singularity instead of a black hole? In the present work we address this problem by studying the scattering of scalar fields on a curved background described by a Reissner-Nordström spacetime with q > m. We discuss the necessary conditions for the well-posedness of the problem, and give some numerical results for low l. The talk "Quasinormal modes from a naked singularity" was presented at the Spanish Relativity Meeting 2012 and was based on the results presented in Chirenti et al. (Phys. Rev. D 86:124008, 2012). © Springer-Verlag Berlin Heidelberg 2014.
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CITATION STYLE
Chirenti, C., Saa, A., & Skákala, J. (2014). Quasinormal Modes from a Naked Singularity. In Springer Proceedings in Mathematics and Statistics (Vol. 60, pp. 179–183). Springer New York LLC. https://doi.org/10.1007/978-3-642-40157-2_20
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