On Higgs and sphaleron effects during the leptogenesis era

被引:89
作者
Nardi, E
Nir, Y
Racker, J
Roulet, E
机构
[1] INFN, Lab Nazl Frascati, I-100044 Frascati, Italy
[2] Univ Antioquia, Inst Fis, Medellin, Colombia
[3] Weizmann Inst Sci, Dept Particle Phys, IL-76100 Rehovot, Israel
[4] Consejo Nacl Invest Cient & Tecn, Ctr Atom Bariloche, RA-8400 San Carlos De Bariloche, Rio Negro, Argentina
关键词
baryogenesis; cosmology of theories beyond the SM;
D O I
10.1088/1126-6708/2006/01/068
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We discuss the effects of various processes that can be active during the leptogenesis era, and present the Boltzmann equations that take them into account appropriately. A non-vanishing Higgs number asymmetry is always present, enhancing the washout of the lepton asymmetry. This is the main new effect when leptogenesis takes place at T > 10(12) GeV, reducing the final baryon asymmetry and tightening the leptogenesis bound on the neutrino masses. If leptogenesis occurs at lower temperatures, electroweak sphalerons partially transfer the lepton asymmetry to a baryonic one, while Yukawa interactions and QCD sphalerons partially transfer the asymmetries of the left-handed fields to the right-handed ones, suppressing the washout processes. Depending on the specific temperature range in which leptogenesis occurs, the final baryon asymmetry can be enhanced or suppressed by factors of order 20% - 40% with respect to the case when these effects are altogether ignored.
引用
收藏
页码:1743 / 1760
页数:18
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