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University of Cambridge > Talks.cam > Isaac Newton Institute Seminar Series > Intrinsic rigidity of extremal horizons and black hole uniqueness
Intrinsic rigidity of extremal horizons and black hole uniquenessAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact nobody. TWT - Twistor theory I will present a recent proof which shows that the intrinsic geometry of compact cross-sections of any vacuum extremal horizon, possibly with a cosmological constant, must admit a Killing vector field. In particular, this implies that the extremal Kerr horizon is the most general such horizon in four-dimensional General Relativity and completes the classification of the associated near-horizon geometries. I will also discuss a recent uniqueness proof which shows that any analytic Einstein spacetime with positive cosmological constant, that contains a static extremal horizon with a maximally symmetric compact cross-section, is the extremal Schwarzschild de Sitter spacetime or its near-horizon geometry. This talk is part of the Isaac Newton Institute Seminar Series series. This talk is included in these lists:
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