Trapped photons in Schwarzschild-Tangherlini spacetimes

preprint2019arXivOpen access

Abstract

We study the set of trapped photons outside the event horizon of Schwarzschild-Tangherlini black holes in dimension d≥4d\geq4. We prove that the only trapped photons are those with constant Boyer-Lindquist coordinate radius. We then identify the set of trapped photons as a submanifold of the tangent bundle of the spacetime, and prove that this submanifold has topology T1Sn−1×R2T^1 S^{n-1}\times \mathbb{R}^2, as suggested in [7].

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