Abstract
Abstract A mechanism for generating baryon density perturbations in the scalar field condensate baryogenesis scenario is proposed. Both the observed baryon asymmetry and the observed periodicity in the large scale structure of the Universe with the characteristic scale 128h −1 Mpc can be explained as due to the evolution of a complex of a complex scalar field condensate formed at the inflationary stage.
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Schedule a callMore From: Astronomical and Astrophysical Transactions, Vol. 33, No. 3
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