Higgs scalar densities and cosmology

Physics – Nuclear Physics

Scientific paper

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Scientific paper

Phase transitions in the early universe are discussed with inclusion of the effects of Higgs scalar chemical potentials as well as fermionic chemical potentials. The conditions for equilibrium, and the critical density to prevent symmetry restoration at high temperatures are studied. It is observed that the decay of pre-existing Higgs scalar asymmetries could greatly reduce baryon number and lepton number to entropy ratios from their initial values.

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