N=2 Supersymmetry and de Sitter space

dc.creatorKallosh, Renata
dc.date2001-09-21
dc.date2001-10-31
dc.date.accessioned2026-07-07T04:12:23Z
dc.date.available2026-07-07T04:12:23Z
dc.descriptionWe present a (unique?) possibility of de Sitter solution in the framework of N=2 supersymmetry (hypersymmetry). We show that a model with a vector and a charged hypermultiplet has a hybrid inflation type potential. It leads to a slow-roll regime in de Sitter type background with all supersymmetries broken spontaneously. Beyond the bifurcation point the waterfall stage abruptly brings the system into a ground state with 2 unbroken supersymmetries. De Sitter stage exists under condition that the superconformal SU(2,2|2) symmetry of the model is softly broken down to N=2 supersymmetry by the vev of the Killing prepotential triplet P^r. This hybrid hypersymmetry model may describe P-term inflation and/or acceleration of the universe at the present epoch.
dc.description24 pages, 5 figs, LaTeX, Improved version
dc.identifierhttps://arxiv.org/abs/hep-th/0109168
dc.identifierhttp://arxiv.org/abs/hep-th/0109168
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/50890
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleN=2 Supersymmetry and de Sitter space
dc.typetext

Files

Collections