Baryon asymmetry and neutrino mixing

被引:184
作者
Buchmuller, W
Plumacher, M
机构
[1] Deutsches Elektronen-Synchrt. DESY
关键词
D O I
10.1016/S0370-2693(96)01232-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In theories where B - L is a spontaneously broken local symmetry, the cosmological baryon asymmetry can be generated by the out-of-equilibrium decay of heavy Majorana neutrinos. We study this mechanism assuming a similar pattern of mixings and masses for leptons and quarks, as suggested by SO(10) unification. This implies that B - L is broken at the unification scale Lambda(GUT) similar to 10(16) GeV, if m(nu mu) similar to 3.10(-3) eV as preferred by the MSW explanation of the solar neutrino deficit. The observed value of the baryon asymmetry, n(B)/s similar to 10(-10), is then obtained without any fine tuning of parameters.
引用
收藏
页码:73 / 77
页数:5
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