In this talk I will present a rigorous construction of examples of black hole formation which are exactly isometric to extremal Reissner--Nordström after finite time.
In particular, our result can be viewed as a definitive disproof of the "third law of black hole thermodynamics.’’ This is based on joint work with Ryan Unger (Princeton).
Christopher Kehle (Zürich): Retiring the third law of black hole thermodynamics
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- Kehle_16_Maerz_2023.pdf 219 KB
