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

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arxiv 0805.4245 v1 pith:ZAJQMTCD submitted 2008-05-28 hep-ph

Shinta Kasuya , Masahiro Kawasaki , Fuminobu Takahashi This is my paper · ORCID
classification hep-ph
keywords fluctuationsisocurvatureaffleck-dinebaryonicconstraintsinflationmechanismmodels
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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.

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  1. Anisotropic Gravitational Waves from Anisotropic Axion Rotation

    hep-ph 2025-08 conditional novelty 6.0 of 10

    A transiently dominant rotating axion sources an induced gravitational wave background whose amplitude and large-scale anisotropy trace the axion's isocurvature fluctuations, with detection prospects for BBO and DECIGO.

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