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Right-handed neutrinos as the source of density perturbations

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arxiv hep-ph/0602052 v1 pith:6SXNQ2Q5 submitted 2006-02-06 hep-ph astro-phhep-th

classification hep-phastro-phhep-th
keywords perturbationsbaryondensitylevelneutrinosright-handedsourceasymmetry
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We study the possibility that cosmological density perturbations are generated by the inhomogeneous decay of right-handed neutrinos. This will occur if a scalar field whose fluctuations are created during inflation is coupled to the neutrino sector. Robust predictions of the model are a detectable level of non-Gaussianity and, if standard leptogenesis is the source of the baryon asymmetry, a baryon isocurvature perturbations at the level of the present experimental constraints.

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