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Cosmo MSW effect for mass varying neutrinos

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arxiv astro-ph/0311131 v2 pith:7O6ZKQVM submitted 2003-11-05 astro-ph hep-ph

Pham Quang Hung (University of Virginia) , Heinrich Päs (Würzburg) This is my paper
classification astro-phhep-ph
keywords neutrinoscosmoeffectmassmassesneutrinovaryingarise
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We consider neutrinos with varying masses which arise in scenarios relating neutrino masses to the dark energy density in the universe. We point out that the neutrino mass variation can lead to level crossing and thus a cosmo MSW effect, having dramatic consequences for the flavor ratio of astrophysical neutrinos.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Visible inelasticity as a probe of tau flavor content of astrophysical neutrinos

    hep-ph 2026-05 unverdicted novelty 7.0 of 10

    Visible inelasticity in starting tracks can statistically separate tau and muon neutrino events, yielding competitive sensitivity to the tau-to-muon flux ratio with current IceCube exposures.

  2. Mass Varying Neutrino Oscillation in Teleparallel Gravity

    hep-ph 2026-06 unverdicted novelty 4.0 of 10

    Torsion-coupled scalar in teleparallel gravity induces density-dependent neutrino masses that alter MSW resonance and yield constraints on coupling parameters from Super-Kamiokande, Borexino and SNO data.

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