Sub-eV Hubble scale inflation within gauge mediated supersymmetry breaking

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dc.creatorAllahverdi, Rouzbeh
dc.creatorJokinen, Asko
dc.creatorMazumdar, Anupam
dc.date2006-10-18
dc.date.accessioned2026-07-07T07:28:16Z
dc.date.available2026-07-07T07:28:16Z
dc.descriptionMinimal Supersymmetric Standard Model with gauge mediated supersymmetry breaking has all the necessary ingredients for a successful sub-eV Hubble scale inflation $H_{\rm inf} \sim 10^{-3}-10^{-1}$ eV. The model generates the right amplitude for scalar density perturbations and a spectral tilt within the range, $0.90 \leq n_s \leq 1$. The reheat temperature is $T_{\rm R} \ls 10$ TeV, which strongly prefers electroweak baryogenesis and creates the right abundance of gravitinos with a mass $m_{3/2} \gs 100$ keV to be the dark matter.
dc.description4 revtex pages
dc.identifierhttps://arxiv.org/abs/hep-ph/0610243
dc.identifierhttp://arxiv.org/abs/hep-ph/0610243
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117672
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleSub-eV Hubble scale inflation within gauge mediated supersymmetry breaking
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