Abstract:
Riemannian Penrose inequality gives the upper bound of the area of the outermost minimal surface in an asymptotically flat space with nonnegative curvature. This inequality shows, roughly speaking, the upper-bound area of black hole horizon, that is, it can be applied in a region with a strong gravitational field. We generalize this inequality so that it can be applied in weak gravitational fields, hence a generalization of Riemannian Penrose inequality.
Areal inequality in weak gravity region
05.09.2025 09:45 - 11:15
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