arXiv Analytics

Sign in

arXiv:astro-ph/9901367AbstractReferencesReviewsResources

Scenario of baryogenesis

D. L. Khokhlov

Published 1999-01-26Version 1

Scenario of baryogenesis is considered in which primordial plasma starting from the Planck scale consists of primordial particles being the precursors of electrons and clusters of particles being the precursors of protons. Equilibrium between the precursors of protons and the precursors of electrons is defined by the proton-electron mass difference. At the temperature equal to the mass of electron, primordial particles transit into protons, electrons, photons.

Related articles: Most relevant | Search more
arXiv:astro-ph/9904306 (Published 1999-04-22)
Improved scenario of baryogenesis
arXiv:astro-ph/0011284 (Published 2000-11-15, updated 2001-03-15)
Electron-Positron Pair Cascades and Precursors in Gamma-Ray Bursts
arXiv:astro-ph/0603839 (Published 2006-03-30, updated 2006-04-20)
The Possible z=0.83 Precursors of z=0 M* Early-type Cluster Galaxies
B. P. Holden et al.