Seminar
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| Location: | UC Berkeley, 60 Evans Hall |
Keywords and Mathematics Subject Classification (MSC)
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Inverse mean curvature flow is a parabolic geometric evolution equation that expands a hypersurface at a rate given by the reciprocal of the mean curvature. In recent years it has proven to be an effective tool in the study problems in general relativity. In this talk I will discuss the role of inverse mean curvature flow in the study of black hole horizons and quasi-local concepts of mass and energy, and outline it's connection to the Penrose Conjecture.
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