Enhancement or damping of fast neutrino flavor conversions due to collisions
Rasmus S. L. Hansen, Shashank Shalgar, Irene Tamborra

TL;DR
This paper investigates how collisions influence fast neutrino flavor conversions in supernovae and merger remnants, revealing that collisions can either enhance or suppress flavor conversion depending on initial angular distributions.
Contribution
It demonstrates the dual role of collisions in either damping or amplifying neutrino flavor conversions based on initial angular configurations.
Findings
Collisions can enhance flavor conversion in isotropic neutrino distributions.
Collisions can suppress flavor conversion in forward-peaked distributions.
The effect of collisions is strongly dependent on initial angular conditions.
Abstract
Fast neutrino flavor conversion can occur in core-collapse supernovae or compact binary merger remnants when non-forward collisions are also at play, and neutrinos are not fully decoupled from matter. This work aims to shed light on the conditions under which fast flavor conversion is enhanced or suppressed by collisions. By relying on a neutrino toy model with three angular bins in the absence of spatial inhomogeneities, we consider two angular configurations: The first one with angular distributions of and that are almost isotropic as expected before complete neutrino decoupling and showing little flavor conversion when collisions are absent. The second one with angular distributions of and that are forward peaked as expected in the free-streaming regime and showing significant flavor conversion in the absence of collisions. By including…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
