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Retiring the third law of black hole thermodynamics

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If you have a question about this talk, please contact Isobel Romero-Shaw.

In this talk I will present a rigorous construction of examples of black hole formation, starting from regular initial data for a self-gravitating charged scalar field, which settle down to extremal Reissner—Nordström in finite advanced time. In particular, our result can be viewed as a definitive disproof of the “third law of black hole thermodynamics.’’ This is joint work with Christoph Kehle.

This talk is part of the DAMTP Friday GR Seminar series.

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