D branes in background fluxes and Nielsen-Olesen instabilities

dc.contributor.authorRusso, J. G. (Jorge Guillermo)
dc.date.accessioned2019-12-10T15:47:21Z
dc.date.available2019-12-10T15:47:21Z
dc.date.issued2016-06-06
dc.date.updated2019-12-10T15:47:21Z
dc.description.abstractIn quantum field theory, charged particles with spin ≥ 1 may become tachyonic in the present of magnetic fluxes above some critical field, signaling an instability of the vacuum. The phenomenon is generic, in particular, similar instabilities are known to exist in open and closed string theory, where a spinning string state can become tachyonic above a critical field. In compactifications involving RR fluxes F p+2, the quantum states which could become tachyonic by the same Nielsen-Olesen mechanism are Dp branes. By constructing an appropriate background with RR magnetic flux that takes into account back-reaction, we identify the possible tachyonic Dp brane states and compute the formula for the energy spectrum in a sector. More generally, we argue that in any background RR magnetic flux, there are high spin Dp quantum states which become very light at critical fields.
dc.format.extent16 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec669243
dc.identifier.issn1126-6708
dc.identifier.urihttps://hdl.handle.net/2445/146385
dc.language.isoeng
dc.publisherSpringer Verlag
dc.relation.isformatofReproducció del document publicat a: https://doi.org/10.1007/JHEP06(2016)021
dc.relation.ispartofJournal of High Energy Physics, 2016, vol. 2016, num. 21
dc.relation.urihttps://doi.org/10.1007/JHEP06(2016)021
dc.rightscc-by (c) Russo, J. G. (Jorge Guillermo), 2016
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationTeoria quàntica de camps
dc.subject.classificationFísica de partícules
dc.subject.otherQuantum field theory
dc.subject.otherParticle physics
dc.titleD branes in background fluxes and Nielsen-Olesen instabilities
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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