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  Fast Neutrino Flavor Conversion: Collective Motion vs. Decoherence

Capozzi, F., Raffelt, G., & Stirner, T. (2019). Fast Neutrino Flavor Conversion: Collective Motion vs. Decoherence. Journal of Cosmology and Astroparticle Physics, 09, 002. Retrieved from https://publications.mppmu.mpg.de/?action=search&mpi=MPP-2019-120.

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 Creators:
Capozzi, Francesco1, Author
Raffelt, Georg1, Author
Stirner, Tobias1, Author
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1Max Planck Institute for Physics, Max Planck Society and Cooperation Partners, ou_2253650              

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Free keywords: Astroparticle Physics
 Abstract: In an interacting neutrino gas, flavor coherence becomes dynamical and can propagate as a collective mode. In particular, tachyonic instabilities can appear, leading to "fast flavor conversion" that is independent of neutrino masses and mixing angles. On the other hand, without neutrino-neutrino interaction, a prepared wave packet of flavor coherence simply dissipates by kinematical decoherence of infinitely many non-collective modes. We reexamine the dispersion relation for fast flavor modes and show that for any wavenumber,there exists a continuum of non-collective modes besides a few discrete collective ones. So for any initial wave packet, both decoherence and collective motion occurs, although the latter typically dominates for a sufficiently dense gas. We derive explicit eigenfunctions for both collective and non-collective modes. If the angular mode distribution of electron-lepton number crosses between positive and negative values, two non-collective modes can merge to become a tachyonic collective mode. We explicitly calculate the interaction strength for this critical point. As a corollary we find that a single crossing always leads to a tachyonic instability. For an even number of crossings, no instability needs to occur.

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 Dates: 2019
 Publication Status: Issued
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Title: Journal of Cosmology and Astroparticle Physics
  Abbreviation : JCAP
Source Genre: Journal
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Pages: - Volume / Issue: 09 Sequence Number: - Start / End Page: 002 Identifier: -