A simple proof of the recent generalisations of Hawking's black hole topology theorem
Istv\'an R\'acz

TL;DR
This paper provides a straightforward, self-contained proof of recent generalizations of Hawking's black hole topology theorem, extending its applicability to higher-dimensional black holes and clarifying the scope of these results.
Contribution
It offers a simple, transparent proof of the recent generalizations of Hawking's theorem to higher dimensions, enhancing understanding of black hole topology.
Findings
Generalized Hawking's topology theorem to higher dimensions
Clarified the applicability range of the theorem
Provided a simple, self-contained proof
Abstract
A key result in four dimensional black hole physics, since the early 1970s, is Hawking's topology theorem asserting that the cross-sections of an "apparent horizon", separating the black hole region from the rest of the spacetime, are topologically two-spheres. Later, during the 1990s, by applying a variant of Hawking's argument, Gibbons and Woolgar could also show the existence of a genus dependent lower bound for the entropy of topological black holes with negative cosmological constant. Recently Hawking's black hole topology theorem, along with the results of Gibbons and Woolgar, has been generalised to the case of black holes in higher dimensions. Our aim here is to give a simple self-contained proof of these generalisations which also makes their range of applicability transparent.
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