Abstract
We discuss the near-singularity region of the linear mass Vaidya metric. In particular, we investigate the structure in the numerical solutions for the scattering of scalar and electromagnetic metric perturbations from the singularity. We observe that, around the total evaporation point, quasinormal-like oscillations appear, indicating that this may be an interesting model for the description of the end point of black hole evaporation.
- Received 29 October 2015
DOI:https://doi.org/10.1103/PhysRevD.94.044035
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