中文

Baryogenesis Below The Electroweak Scale

高能物理 - 唯象学 2009-10-31 v1 天体物理学 高能物理 - 理论

摘要

We propose a new alternative for baryogenesis which resolves a number of the problems associated with GUT and electroweak scenarios, and which may allow baryogenesis even in modest extensions of the standard model. If the universe never reheats above the electroweak scale following inflation, GUT baryon production does not occur and at the same time thermal sphalerons, gravitinos and monopoles are not produced in abundance. Nevertheless, non-thermal production of sphaleron configurations via preheating could generate the observed baryon asymmetry of the universe.

关键词

引用

@article{arxiv.hep-ph/9902420,
  title  = {Baryogenesis Below The Electroweak Scale},
  author = {Lawrence M. Krauss and Mark Trodden},
  journal= {arXiv preprint arXiv:hep-ph/9902420},
  year   = {2009}
}

备注

4 pages, revtex, submitted to PRL