Universal Thermal Instabilities and the High-Temperature Phase of the N=4 Superstrings

dc.creatorKounnas, Costas
dc.date1999-02-10
dc.date.accessioned2026-07-07T04:25:57Z
dc.date.available2026-07-07T04:25:57Z
dc.descriptionUsing the properties of gauged N=4 supergravity, we show that it is possible to derive a universal thermal effective potential that describes all possible high-temperature instabilities of the known N=4 superstrings. These instabilities are due to non-perturbative dyonic modes, which become tachyonic in a region of the thermal moduli space M={s,t,u}; M is common to all non-perturbative dual-equivalent N=4 superstrings in five dimensions. We analyse the non-perturbative thermal potential and show the existence of a phase transition at high temperatures corresponding to a condensation of 5-branes. This phase is described in detail, using an effective non-critical string theory.
dc.description15 pages, LATEX file, no figures
dc.identifierhttps://arxiv.org/abs/hep-th/9902072
dc.identifierhttp://arxiv.org/abs/hep-th/9902072
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/55932
dc.subjectHigh Energy Physics - Theory
dc.titleUniversal Thermal Instabilities and the High-Temperature Phase of the N=4 Superstrings
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