Titlebook: Large Scale Structure and Motions in the Universe; Proceeding of an Int M. Mezzetti,G. Giuricin,M. Ramella Conference proceedings 1989 Kluw

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Inflation and the Baryon Isocurvature Modelns are assumed to have come from dilution of the primeval baryon to entropy ratio by decay of a massive field produced as quantum fluctuations leaving the horizon during the inflation era. This scenario requires an expansion time history that would be produced by a model inflaton field that has nega

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Titlebook: Large Scale Structure and Motions in the Universe; Proceeding of an Int M. Mezzetti,G. Giuricin,M. Ramella Conference proceedings 1989 Kluw

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