Are cosmological energies and processes realized in local astrophysical events?

Abstract

If the processes of baryogenesis and leptogenesis were realized at energies less than 5·10²⁰eV, then they should be carried out in modern high-energy astrophysical processes. But this means a constant violation of the law of conservation of baryon and lepton numbers and the stability of protons. Therefore, we propose the principle of energy prohibition, according to which in astrophysical and experimental local processes in a cosmologically stable vacuum it is impossible to achieve energies at which violations of the baryon and lepton numbers, the maximum energies of the Big Bang after inflation, such as the decay energy of inflaton, can occur. In turn, this imposes lower restrictions on the heating energy after inflation associated with baryogenesis, E≥10^21.5–22eV. Therefore, all models of baryogenesis at energies below 5·10²⁰eV, proposed by a number of authors, need to be revised.