Improved scenario of baryogenesis

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dc.creatorKhokhlov, D. L.
dc.date1999-04-22
dc.date.accessioned2026-07-07T02:31:20Z
dc.date.available2026-07-07T02:31:20Z
dc.descriptionIt 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.
dc.description3 pages LaTeX
dc.identifierhttps://arxiv.org/abs/astro-ph/9904306
dc.identifierhttp://arxiv.org/abs/astro-ph/9904306
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14121
dc.subjectAstrophysics
dc.titleImproved scenario of baryogenesis
dc.typetext

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