Cosmological Avatars of the Landscape I: Bracketing the SUSY Breaking Scale

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dc.creatorHolman, R.
dc.creatorMersini-Houghton, L.
dc.creatorTakahashi, Tomo
dc.date2006-11-21
dc.date.accessioned2026-07-07T11:23:12Z
dc.date.available2026-07-07T11:23:12Z
dc.descriptionWe investigate the effects of quantum entanglement between our horizon patch and others due to the tracing out of long wavelength modes in the wavefunction of the Universe as defined on a particular model of the landscape. In this, the first of two papers devoted to this topic, we find that the SUSY breaking scale is bounded both above {\em and} below: $10^{-10} M_{\rm P}\leq M_{\rm SUSY}\leq 10^{-8} M_{\rm P}$ for $GUT$ scale inflation. The lower bound is at least five orders of magnitude larger than the expected value of this parameter and can be tested by LHC physics.
dc.description7 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/hep-th/0611223
dc.identifierhttp://arxiv.org/abs/hep-th/0611223
dc.identifierPhys.Rev.D77:063510,2008
dc.identifierdoi:10.1103/PhysRevD.77.063510
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194815
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleCosmological Avatars of the Landscape I: Bracketing the SUSY Breaking Scale
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