Damping rates in the MSSM and electroweak baryogenesis

被引:19
|
作者
Elmfors, P
Enqvist, K
Riotto, A
Vilja, I
机构
[1] Univ Stockholm, Dept Phys, S-11385 Stockholm, Sweden
[2] Univ Helsinki, Dept Phys, FIN-00014 Helsinki, Finland
[3] Univ Helsinki, Helsinki Inst Phys, FIN-00014 Helsinki, Finland
[4] CERN, Div Theory, CH-1211 Geneva 23, Switzerland
[5] Turku Univ, Dept Phys, FIN-20014 Turku, Finland
基金
芬兰科学院;
关键词
D O I
10.1016/S0370-2693(99)00169-0
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an analysis of the thermalization rate of Higgsinos and wines based on the imaginary part of the two-point Green function in the 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 gamma((H) over tilde)similar or equal to 0.025T, gamma((W) over tilde)similar or equal to 0.065T. The contribution from scattering with scalars is relatively small. Implications for baryogenesis are also discussed. (C) 1999 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:279 / 286
页数:8
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