Big Bang Baryogenesis
高能物理 - 唯象学
2015-06-25 v1 天体物理学
摘要
An overview of baryogenesis in the early Universe is presented. The standard big bang model including big bang nucleosynthesis and inflation is breifly reviewed. Three basic models for baryogenesis will be developed: The ``standard" out-of-equilibrium decay model; the decay of scalar consensates along flat directions in supersymmetric models; and lepto-baryogenesis, which is the conversion of a lepton asymmetry into a baryon asymmetry via non-perturbative electroweak interactions.
引用
@article{arxiv.hep-ph/9404352,
title = {Big Bang Baryogenesis},
author = {Keith A. Olive},
journal= {arXiv preprint arXiv:hep-ph/9404352},
year = {2015}
}
备注
36 pages, LaTeX, UMN-TH-1249, Lectures given at the 33rd International Winter School on Nuclear and Particle Physics, ``Matter Under Extreme Conditions", Feb. 27 - March 5 1994, Schladming Austria