Supergravity, M theory and Cosmology

dc.creatorKallosh, Renata
dc.date2002-05-30
dc.date.accessioned2026-07-07T04:13:37Z
dc.date.available2026-07-07T04:13:37Z
dc.descriptionWe discuss some recent attempts to reconcile cosmology with supergravity and M/string theory. First of all, we point out that in extended supergravities the scalar masses are quantized in terms of the cosmological constant in de Sitter vacua: the eigenvalues of the Casimir operator 3 m^2/Λtake integer values. For the current value of the cosmological constant extended supergravities predict ultra light scalars with the mass of the order of Hubble constant, 10^{-33} eV. This may have interesting consequences for cosmology. Turning our attention to cosmological implications of M/string theory, we present a possibility to use string theory D-brane constructions to reproduce the main features of hybrid inflation. We stress an important role played by Fayet-Iliopoulos terms responsible for the positive contribution to the potentials and stabilization of moduli.
dc.description24 pages, a talk at Stephen Hawking's 60th birthday conference, Cambridge University, Jan. 2002
dc.identifierhttps://arxiv.org/abs/hep-th/0205315
dc.identifierhttp://arxiv.org/abs/hep-th/0205315
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51327
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSupergravity, M theory and Cosmology
dc.typetext

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