Transitions Between Flux Vacua

dc.creatorde Alwis, S. P.
dc.date2006-05-18
dc.date2006-11-03
dc.date.accessioned2026-07-07T10:42:20Z
dc.date.available2026-07-07T10:42:20Z
dc.descriptionA dynamical description of the transitions between different backgrounds requires the existence of a background independent action which propagates the correct number of degrees of freedom and couples bulk supergravity to certain higher dimensional branes. We present classical equations for configurations that separate the world into regions with different flux parameters etc. and discuss the difficulties of trying to construct an action that describes the transitions between them within the framework of supergravity.
dc.descriptionType IIA anomaly resolved, added appendix B reference added
dc.identifierhttps://arxiv.org/abs/hep-th/0605184
dc.identifierhttp://arxiv.org/abs/hep-th/0605184
dc.identifierPhys.Rev.D74:126010,2006
dc.identifierdoi:10.1103/PhysRevD.74.126010
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181914
dc.subjectHigh Energy Physics - Theory
dc.titleTransitions Between Flux Vacua
dc.typetext

Files

Collections