Please use this identifier to cite or link to this item: https://olympias.lib.uoi.gr/jspui/handle/123456789/16352
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dc.contributor.authorKanti, P.en
dc.contributor.authorMavromatos, N. E.en
dc.contributor.authorRizos, J.en
dc.contributor.authorTamvakis, K.en
dc.contributor.authorWinstanley, E.en
dc.date.accessioned2015-11-24T18:30:14Z-
dc.date.available2015-11-24T18:30:14Z-
dc.identifier.issn0556-2821-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16352-
dc.rightsDefault Licence-
dc.subjectarbitrary gauge groupsen
dc.subjectyang-mills solitonsen
dc.subjectno-hairen
dc.subjectinstabilityen
dc.subjectsphaleronsen
dc.subjectsystemsen
dc.subjectnumberen
dc.titleDilatonic black holes in higher curvature string gravity. II. Linear stabilityen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.secondary<Go to ISI>://000073767400034-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate1998-
heal.abstractWe demonstrate the linear stability of dilatonic black holes appearing in a string-inspired higher-derivative gravity theory with a Gauss-Bonnet curvature-squared term. The proof is accomplished by mapping the system to a one-dimensional Schrodinger problem which admits no bound states. This result is important in that it constitutes a linearly stable example of a black hole that bypasses the "no-hair conjecture." However, dilaton hair is secondary in the sense that it is not accompanied by any new quantum number for the black hole solution.en
heal.journalNamePhysical Review Den
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)



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