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Model for Fluctuating Inflaton Coupling: Sneutrino Induced Adiabatic Perturbations and Nonthermal Leptogenesis

2003/06/30 by Anupam Mazumdar · 2 citations
Earth and Planetary Sciences · Physics and Astronomy · #Cosmology and Gravitation Theories #Geophysics and Gravity Measurements #Solar and Space Plasma Dynamics #astro-ph #hep-ph

paper · pdf · doi:10.1103/physrevlett.92.241301

published as Phys.Rev.Lett. 92 (2004) 241301 · 4 pages, version to be published in PRL

arxiv created 2004/03/26 · openalex publication_date 2004/06/15 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We discuss a unique possibility of generating adiabatic density perturbations and leptogenesis from the spatial fluctuations of the inflaton decay rate. The key assumption is that the initial isocurvature perturbations are created in the right-handed sneutrino sector during inflation which is then converted into adiabatic perturbations when the inflaton decays. We discuss distinct imprints on the cosmic microwave background radiation, which can distinguish nonthermal versus thermal leptogenesis.

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