Calculation of cosmological baryon asymmetry in grand unified gauge models

Physics – Nuclear Physics

Scientific paper

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Scientific paper

Features of grand unified gauge models relevant to cosmology are discussed. Several SU(5) and SO(10) models are considered in detail. Boltzmann transport equation methods are used to calculate the development of baryon asymmetry in the early universe. Comparison with observation places constraints on possible grand unified models.
Work supported in part by the US Department of Energy under contract no. DE-AC-03-79ER0068 and by the Fleischmann foundation.

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