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arxiv: hep-ph/0012291 · v1 · submitted 2000-12-21 · ✦ hep-ph · astro-ph

Creation of large spatial fluctuations in neutrino asymmetry by neutrino oscillations

classification ✦ hep-ph astro-ph
keywords asymmetryneutrinofluctuationsgrowthlargeoscillationsspacespatial
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We consider active-sterile neutrino oscillations in the early universe in an inhomogeneous isocurvature background. We show that very small initial baryonic seed-inhomogeneities can trigger a growth of very large amplitude spatial fluctuations in lepton asymmetry. Domains of varying asymmetry are observed to persist for a long time despite dissipative effects. The space dependent asymmetry profiles give rise to MSW-resonances within the domain boundaries, enhancing dramatically the equilibration of the sterile neutrino species. According to our one-dimensional toy-model, the effect is so strong that almost the entire parameter space where exponential growth of asymmetry occurs would be ruled out by nucleosynthesis.

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