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Systematic local simulations of fast neutrino flavor conversions with scattering effects

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arxiv 2402.04741 v2 pith:THAKT4E6 submitted 2024-02-07 hep-ph astro-ph.HE

classification hep-phastro-ph.HE
keywords flavorconversionsfastmodelmodelsneutrinocollisionalmomentum
verification ladder T0 review T1 audit T2 compute T3 formal
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We investigate the dynamics of fast neutrino flavor conversions (FFCs) in the one-dimensional (1D) and zero-dimensional (0D) models, in which spatial advection is considered and ignored, respectively. In this study, we employ snapshots obtained by our self-consistent, realistic Boltzmann-neutrino-radiation-hydrodynamics simulations. We show that the FFC growth rate is considerably larger in the 1D model than in the 0D model, as expected from the previous linear analysis results. We find that the momentum space dimension does not significantly influence the neutrino transition probability in 1D models. On the other hand, in the 0D model without collisions, the FFC depends on the momentum space, and the azimuthal angle dependence breaks the periodicity of the FFC. Our study demonstrates that collisional instability can lead to further flavor conversions on a long time scale in 1D models after the asymptotic state of FFC has been reached. Such an effect should be taken into consideration when the fast and collisional flavor instabilities coexist.

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

  1. Three-dimensional core-collapse supernova models with phenomenological treatment of neutrino flavor conversions

    astro-ph.HE 2025-01 conditional novelty 5.0 of 10

    Three-dimensional supernova simulations with imposed neutrino flavor equipartition raise the explosion energy to about 10^51 erg and change predicted neutrino and gravitational wave signals.

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