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Isocurvature fluctuations in Affleck-Dine mechanism and constraints on inflation models

We reconsider the Affleck-Dine mechanism for baryogenesis and show that the baryonic isocurvature fluctuations are generated in many inflation models in supergravity. The inflationary scale and the reheating temperature must satisfy certain constraints to avoid too large baryonic isocurvature fluctuations.

preprint2008arXivOpen access
Shinta KasuyaMasahiro KawasakiFuminobu Takahashi
hep-ph
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Open access3 authors1 topic
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Shinta KasuyaMasahiro KawasakiFuminobu Takahashi

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