On the W-hair of String Black Holes and the Singularity Problem

dc.creatorEllis, John
dc.creatorMavromatos, N. E.
dc.creatorNanopoulos, D. V.
dc.date1992-04-29
dc.date.accessioned2026-07-07T04:18:45Z
dc.date.available2026-07-07T04:18:45Z
dc.descriptionWe argue that the infinitely many gauge symmetries of string theory provide an infinite set of conserved (gauge) quantum numbers (W-hair) which characterise black hole states and maintain quantum coherence, even during exotic processes like black hole evaporation/decay. We study ways of measuring the W-hair of spherically-symmetric four-dimensional objects with event horizons, treated as effectively two-dimensional string black holes. Measurements can be done either through the s-wave scattering of light particles off the string black-hole background, or through interference experiments of Aharonov-Bohm type. We also speculate on the role of the extended W-symmetries possessed by the topological field theories that describe the region of space-time around a singularity.
dc.description19 pages
dc.identifierhttps://arxiv.org/abs/hep-th/9204096
dc.identifierhttp://arxiv.org/abs/hep-th/9204096
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/53315
dc.subjectHigh Energy Physics - Theory
dc.titleOn the W-hair of String Black Holes and the Singularity Problem
dc.typetext

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