Improved scenario of baryogenesis
Astrophysics
2007-05-23 v1
Abstract
It is assumed that, in the primordial plasma, at the temperatures above the mass of electron, fermions are in the neutral state being the superposition of particle and antiparticle. There exists neutral proton-electron symmetry. Proton-electron equilibrium is defined by the proton-electron mass difference. At the temperature equal to the mass of electron, pairs of neutral electrons annihilate into photons, and pairs of neutral protons and electrons survive as protons and electrons.
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Cite
@article{arxiv.astro-ph/9904306,
title = {Improved scenario of baryogenesis},
author = {D. L. Khokhlov},
journal= {arXiv preprint arXiv:astro-ph/9904306},
year = {2007}
}
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