SUPERSYMMETRIC (S)NEUTRINO-MASS INDUCED BARYOGENESIS

被引:20
作者
CAMPBELL, BA
DAVIDSON, S
OLIVE, KA
机构
[1] UNIV CALIF BERKELEY,CTR PARTICLE ASTROPHYS,BERKELEY,CA 94720
[2] UNIV MINNESOTA,DEPT PHYS & ASTRON,MINNEAPOLIS,MN 55455
关键词
D O I
10.1016/0370-2693(93)90044-I
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We propose a new mechanism for baryogenesis in supersymmetric extensions of the standard model, that does no depend on (super)GUT interactions. It occurs by the non-perturbative electroweak reprocessing of a lepton asymmetry. This lepton asymmetry is generated by the effects of lepton number violating induced operators, arising from ''see-saw'' (s)neutrino masses, which act on scalar condensate oscillations along flat directions of the supersymmetric standard model.
引用
收藏
页码:63 / 67
页数:5
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