Neutrino quantum kinetics in two spatial dimensions
Marie Cornelius, Shashank Shalgar, Irene Tamborra

TL;DR
This paper models neutrino flavor evolution in two spatial dimensions, incorporating collisions, advection, and perturbations, revealing complex flavor conversion patterns that are crucial for understanding astrophysical phenomena.
Contribution
It introduces a (2+1+1) dimensional simulation of neutrino quantum kinetics, including collisions and perturbations, advancing beyond spherically symmetric models.
Findings
Flavor conversion is significantly affected by perturbations.
Neutrino advection spreads flavor waves across regions.
Symmetry breaking leads to alternating flavor conversion regions.
Abstract
Our understanding of neutrino flavor conversion in the innermost regions of core-collapse supernovae and neutron star mergers is mostly limited to spherically symmetric configurations that facilitate the numerical solution of the quantum kinetic equations. In this paper, we simulate neutrino quantum kinetics within a (2+1+1) dimensional setup: we model the flavor evolution during neutrino decoupling from matter in two spatial dimensions, one neutrino momentum variable, and time; taking into account non-forward neutral current and charged current collisions of neutrinos with the matter background, as well as neutrino advection. In order to mimic fluctuations in the neutrino emission and matter background, and explore their effect on the flavor evolution, we introduce perturbations in the collision term as well as in the vacuum term of the Hamiltonian. Because of such perturbations, the…
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Taxonomy
TopicsNeutrino Physics Research · Dark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies
