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Aharonov-Bohm protection of black hole's baryon/skyrmion hair

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arxiv 1611.09370 v1 pith:7RYXX7IN submitted 2016-11-28 hep-th astro-ph.HEgr-qchep-ph

classification hep-thastro-ph.HEgr-qchep-ph
keywords baryonblackskyrmionnumberholeaharonov-bohmcertainclassical
verification ladder T0 review T1 audit T2 compute T3 formal
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The baryon/skyrmion correspondence implies that the baryon number is encoded into a topological surface integral. Under certain conditions that we clarify, this surface integral can be measured by an asymptotic observer in form of an Aharonov-Bohm phase-shift in an experiment in which the skyrmion passes through a loop of a probe string. In such a setup the baryon/skyrmion number must be respected by black holes, despite the fact that it produces no long-range classical field. If initially swallowed by a black hole, the baryon number must resurface in form of a classical skyrmion hair, after the black hole evaporates below a certain critical size. Needless to say, the respect of the baryon number by black holes is expected to have potentially-interesting astrophysical consequences.

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