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University of Cambridge > Talks.cam > DAMTP Friday GR Seminar > On the third law of black hole mechanics for supersymmetric black holes
On the third law of black hole mechanics for supersymmetric black holesAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Daniela Cors. Recently it has been shown that the third law of black hole mechanics can be violated: an exactly extremal Reissner-Nordström black hole can form in finite time in gravitational collapse of matter with a large charge to mass ratio. However, it has also been proved that this cannot happen if the matter satisfies a “supersymmetric” lower bound on its energy in terms of its charge. In this talk, I will discuss these developments, as well as extensions of this latter proof to supersymmetric black holes with a negative cosmological constant and for such black holes (with non-positive cosmological constant) not formed in collapse. The proofs of these results rely on ideas related to quasi-local energy and proofs of the positive energy theorems: these shall be discussed, and the main theorem given as a rigidity result associated with the interior of a “supersymmetric surface” – a concept to be introduced. This talk is part of the DAMTP Friday GR Seminar series. This talk is included in these lists:
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