TY - JOUR
T1 - Aharonov–Bohm protection of black hole's baryon/skyrmion hair
AU - Dvali, Gia
AU - Gußmann, Alexander
N1 - Funding Information:
The work of G.D. was supported by Humboldt Foundation under Alexander von Humboldt Professorship, by European Commission under ERC Advanced Grant 339169 “Selfcompletion”, by DFG SFB/TRR 33 “The Dark Universe” and by the DFG cluster of excellence EXC 153 “Origin and Structure of the Universe”. The work of A.G. was supported by the DFG cluster of excellence EXC 153 “Origin and Structure of the Universe” and by Humboldt Foundation.
Publisher Copyright:
© 2017 The Author(s)
PY - 2017/5/10
Y1 - 2017/5/10
N2 - 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.
AB - 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.
KW - Aharonov–Bohm effect
KW - Black hole
KW - Black hole hair
KW - Skyrmion
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U2 - 10.1016/j.physletb.2017.03.004
DO - 10.1016/j.physletb.2017.03.004
M3 - Article
AN - SCOPUS:85015008421
SN - 0370-2693
VL - 768
SP - 274
EP - 279
JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
ER -