Extensible Black Hole Embeddings for Apparently Forbidden Periodicities

Abstract

Imposing extendibility on Kasner-Fronsdal black hole local isometric embedding is equivalent to removing conic singularities in Kruskal representation. Allowing for globally non-trivial (living in M5× S1) embeddings, parameterized by k, extendibility can be achieved for apparently forbidden frequencies ω1(k)ω (k) ω2(k). The Hawking-Gibbons limit, say ω1,2(0)= 14M for Schwarzschild geometry, is respected. The corresponding Kruskal sheets are viewed as slices in some Kaluza-Klein background. Euclidean k discreteness, dictated by imaginary time periodicity, is correlated with twistor flux quantization.

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