Damping rates in the MSSM and electroweak baryogenesis

dc.creatorElmfors, Per
dc.creatorEnqvist, Kari
dc.creatorRiotto, Antonio
dc.creatorVilja, Iiro
dc.date1998-09-25
dc.date.accessioned2026-07-07T10:33:44Z
dc.date.available2026-07-07T10:33:44Z
dc.descriptionWe present an analysis of the thermalization rate of Higgsinos and winos based on the imaginary part of the two-point Green function in the {\it unbroken} phase of the MSSM. We use improved propagators including resummation of hard thermal loops and the thermalization rate is computed at the one-loop level in the high temperature approximation. We find that the damping is typically dominated by scattering with gauge bosons, resulting in a damping rate of about $γ_{\Ht}\simeq 0.025T$, $γ_{\Wt}\simeq 0.065T$. The contribution from scattering with scalars is relatively small. Implications for baryogenesis are also discussed.
dc.description10 pages LaTEX, 1 ps figure
dc.identifierhttps://arxiv.org/abs/hep-ph/9809529
dc.identifierhttp://arxiv.org/abs/hep-ph/9809529
dc.identifierPhys.Lett.B452:279-286,1999
dc.identifierdoi:10.1016/S0370-2693(99)00169-0
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179224
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDamping rates in the MSSM and electroweak baryogenesis
dc.typetext

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