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).
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References
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Acknowledgements
This work was supported by FAPESP, CNPq and the Max Planck Society.
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Chirenti, C., Saa, A., Skákala, J. (2014). Quasinormal Modes from a Naked Singularity. In: García-Parrado, A., Mena, F., Moura, F., Vaz, E. (eds) Progress in Mathematical Relativity, Gravitation and Cosmology. Springer Proceedings in Mathematics & Statistics, vol 60. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-40157-2_20
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DOI: https://doi.org/10.1007/978-3-642-40157-2_20
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