中文

Leptogenesis with cosmic strings

高能物理 - 唯象学 2007-05-23 v1

摘要

A new scenario for baryogenesis is described. The basic idea is that theories beyond the standard model which contain a U(1)BL{\rm U}(1)_{B-L} gauge symmetry, where BB and LL are respectively baryon and lepton numbers, predict the existence of BLB-L cosmic strings with right-handed neutrinos trapped as transverse zero modes. Cosmic string loops loose their energy via gravitational radiation and rapidly decay releasing these right-handed neutrinos. These decay into lepton and electroweak Higgs boson producing an initial lepton asymmetry. This lepton asymmetry is then converted into a baryon asymmetry via sphaleron transitions. The minimal extension of the standard model and the minimal grand unified theory for which this scenario works are respectively SU(3)c×SU(2)L×U(1)R×U(1)BL{\rm SU}(3)_c \times {\rm SU}(2)_L \times {\rm U}(1)_R \times {\rm U}(1)_{B-L} and SO(10).

关键词

引用

@article{arxiv.hep-ph/9802333,
  title  = {Leptogenesis with cosmic strings},
  author = {R. Jeannerot},
  journal= {arXiv preprint arXiv:hep-ph/9802333},
  year   = {2007}
}

备注

Published in the Proceedings of the XXXIInd Rencontres de Moriond on ``Electroweak Interactions and Unified Theories'', Les Arcs, Savoie, France, March 15-22, 1997