SUSY-GUTs, SUSY-Seesaw and the Neutralino Dark Matter

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dc.creatorCalibbi, L.
dc.creatorMambrini, Y.
dc.creatorVempati, S. K.
dc.date2007-04-26
dc.date2007-09-17
dc.date.accessioned2026-07-07T12:23:51Z
dc.date.available2026-07-07T12:23:51Z
dc.descriptionWe will consider a SUSY-SU(5) with one right-handed neutrino with a large top like Yukawa coupling. Assuming universal soft masses at high scale we compute the low-energy spectrum and subsequently the neutralino LSP relic density taking also into consideration SU(5) as well as the see-saw running effects above the gauge coupling unification scale. We found that there exists no viable region in parameter space for $\tanβ\ler ~35$. The $\tildeτ$ coannihilation process starts becoming efficient for $\tanβ\ger 35-40$. However, this process is significantly constrained by the limited range in which the stau is lighter than the neutralino. In fact, for a given $\tanβ$ we find that there exists an upper bound on the lightest neutralino mass ($M_{χ_1^0}$) in this region. The A-pole funnel region appears at very large $\tanβ\simeq 45-50$, while the focus-point region does not make an appearance till large ($m_0,M_{1/2}$), namely a few TeV. Large $A_0$ terms at high scale can lead to extended regions consistent with WMAP constraints and remove the upper bounds in the stau coannihilation regions.
dc.description18 pages, 7 figures; references added, figure added, improved discussions in text, to appear in JHEP
dc.identifierhttps://arxiv.org/abs/0704.3518
dc.identifierhttp://arxiv.org/abs/0704.3518
dc.identifierJHEP 0709:081,2007
dc.identifierdoi:10.1088/1126-6708/2007/09/081
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/214140
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleSUSY-GUTs, SUSY-Seesaw and the Neutralino Dark Matter
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