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- W3100288295 abstract "We introduce the concept of a geometric horizon, which is a surface distinguished by the vanishing of certain curvature invariants which characterize its special algebraic character. We motivate its use for the detection of the event horizon of a stationary black hole by providing a set of appropriate scalar polynomial curvature invariants that vanish on this surface. We extend this result by proving that a non-expanding horizon, which generalizes a Killing horizon, coincides with the geometric horizon. Finally, we consider the imploding spherically symmetric metrics and show that the geometric horizon identifies a unique quasi-local surface corresponding to the unique spherically symmetric marginally trapped tube, implying that the spherically symmetric dynamical black holes admit a geometric horizon. Based on these results, we propose a suite of conjectures concerning the application of geometric horizons to more general dynamical black hole scenarios." @default.
- W3100288295 created "2020-11-23" @default.
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- W3100288295 date "2017-12-21" @default.
- W3100288295 modified "2023-09-25" @default.
- W3100288295 title "Identification of black hole horizons using scalar curvature invariants" @default.
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- W3100288295 doi "https://doi.org/10.1088/1361-6382/aa9804" @default.
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