Improved scenario of baryogenesis

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. Standard scenario of baryogenesis occurs as follows [1]. In the thermodynamically equilibrium primordial plasma, all the particles with m ≤ T exist in equal abundances per spin degree of freedom. This means that, at T > mp, there exist approximately equal abundances of protons p and antiprotons p̄. Excess of baryonic charge arises in the processes of X, Ybosons decays under the following conditions: non-conservation of the baryonic charge and CP-violation. At T < mp, pp̄ annihilate, with the excess of p survives. Let us consider another scenario of baryogenesis. Let us assume that, in the primordial plasma, at T > me, fermions are in the neutral state being the superposition of particle and antiparticle |ψ >= 1 √ 2 (ψ̄ + ψ). (1) Neutral electrons are in the state being the superposition of electron and positron |e >= 1 √ 2 (e− + e). (2) Neutral protons are in the state being the superposition of proton and antiproton |p >= 1 √ 2 (p̄+ p). (3) Let us assume that, at T > me, there exists neutral proton-electron symmetry. For the neutral electron, the sequence of spin transformations ↑↓↑↓↑ transits the particle into itself. Let us identify the cluster of neutral electrons ↑↓↑↓↑ with the neutral proton. The probability of finding such a cluster is given by