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arXiv · 2608.02984

Neutrino flavor-wave transport: Numerical tests and theoretical challenges

Abstract

Neutrino quantum kinetics is computationally intractable in the neutrino-dense arenas of core-collapse supernovae and neutron star mergers. Flavor-wave (or flavomon) transport is an emerging approach to this problem in which small-scale flavor inhomogeneities are treated as quasiparticles with properties determined by the local mean background. We present the first numerical calculations of flavor-wave transport under slow driving. Our results show some quantitative successes but also underscore the theoretical challenges that need to be overcome. Two issues are particularly concerning. (1) Nonlinear wave-wave coupling may be important. (2) Degeneracies and small energy gaps are responsible for significant nonadiabatic transitions. Future work will need to address these points if flavor-wave transport is to be viable in settings of astrophysical interest. Other topics examined include flavor-wave parallel transport and flavor-space symmetry breaking.

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BibTeXRIS

Anson Kost, Lucas Johns, Huaiyu Duan. 2026-08-04. Neutrino flavor-wave transport: Numerical tests and theoretical challenges. https://arxiv.org/abs/2608.02984

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