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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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Palmerston Room, Fisher Building, St Johns College https://cl-cam-ac-uk.zoom.us/j/4361570789?pwd=Nkl2T3ZLaTZwRm05bzRTOUUxY3Q4QT09&from=addon Webinar & FW11, Computer Laboratory, William Gates Building.

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