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Baryon Isocurvature Perturbation in the Affleck-Dine Baryogenesis mechanism

Kazuya Koyama, Jiro Soda

astro-pharXiv:astro-ph/9810006

Abstract

We propose a primeval baryon isocurvature model in the context of the Affleck-Dine (AD) baryogenesis mechanism. Quantum fluctuations of the AD field during inflation produce fluctuations in the baryon number. We obtain a model which gives both the appropriate baryon to entropy ratio of the order 10-11 and the gaussian baryon isocurvature perturbation of the order 10-3 at the break of the spectrum 1 Mpc with the steep spectrum n=-1.5 on large scales >1 Mpc.

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