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Hagedorn transition and chronology protection in string theory

dc.contributor.authorCosta, Miguel S.
dc.contributor.authorHerdeiro, Carlos A.R.
dc.contributor.authorPenedones, J.
dc.contributor.authorSousa, Nuno
dc.date.accessioned2010-06-16T11:44:44Z
dc.date.available2010-06-16T11:44:44Z
dc.date.issued2005
dc.description.abstractWe conjecture chronology is protected in string theory due to the condensation of light winding strings near closed null curves. This condensation triggers a Hagedorn phase transition, whose end-point target space geometry should be chronological. Contrary to conventional arguments, chronology is protected by an infrared effect. We support this conjecture by studying strings in the O-plane orbifold, where we show that some winding string states are unstable and condense in the non-causal region of spacetime. The oneloop string partition function has infrared divergences associated to the condensation of these states.pt
dc.description.versionpeerreviewed
dc.identifier.citationCosta, Miguel S. [et al.] - Hagedorn transition and chronology protection in string theory. "Nuclear Physics B" [Em linha]. ISSN: 0550-3213. Vol. 728, nº 1-3 (Set. 2005), p. 148-178pt
dc.identifier.issn0550-3213
dc.identifier.urihttp://hdl.handle.net/10400.2/1519
dc.language.isoengpt
dc.publisherElsevierpt
dc.relation.publisherversiondoi:10.1016/j.nuclphysb.2005.08.022pt
dc.subjectTeoria de cordaspt
dc.subjectProteção de cronologiapt
dc.subjectTransição de Hagedornpt
dc.subjectOrbivariedadespt
dc.titleHagedorn transition and chronology protection in string theorypt
dc.typejournal article
dspace.entity.typePublication
oaire.citation.endPage178pt
oaire.citation.startPage148pt
oaire.citation.titleNuclear Physics Bpt
person.familyNameSousa
person.givenNameNuno
person.identifier.ciencia-idE914-E920-B2A0
person.identifier.orcid0000-0002-2681-5035
person.identifier.ridF-5307-2014
person.identifier.scopus-author-id7003438443
rcaap.rightsopenAccesspt
rcaap.typearticlept
relation.isAuthorOfPublication0d49a6e8-e597-4edf-a203-a426d69abd77
relation.isAuthorOfPublication.latestForDiscovery0d49a6e8-e597-4edf-a203-a426d69abd77

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