Neutrino propagation hinders fast pairwise flavor conversions
Shashank Shalgar, Ian Padilla-Gay, Irene Tamborra

TL;DR
This study demonstrates that the advective motion of neutrinos suppresses rapid pairwise flavor conversions unless conditions are sustained over longer timescales, significantly affecting models of astrophysical phenomena.
Contribution
We provide the first detailed numerical analysis of neutrino flavor evolution in a multi-dimensional setup including advection, revealing its suppressive effect on fast flavor conversions.
Findings
Advective terms hinder pairwise flavor conversions under certain conditions.
Fast conversions require sustained, global conditions like LESA.
Linear stability analysis has critical limitations in predicting flavor instabilities.
Abstract
Neutrino flavor conversions may dramatically affect the inner working of compact astrophysical objects as well as the synthesis of the heavier elements. We present the first sophisticated numerical solution of the neutrino flavor conversion within a (2+1+1) dimensional setup: we include the advective term in the neutrino equations of motion and track the flavor evolution in two spatial dimensions, one angular variable, and time. Notably, the advective term hinders the development of neutrino pairwise conversions, if the conditions favoring such conversions (i.e., crossings between the angular distributions of and or a non-negligible flux of neutrinos traveling backward with respect to the main propagation direction) exist for time scales shorter than the typical time scale of the advective term. As a consequence, fast pairwise conversions can only occur when the…
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