Fast Neutrino-Flavor Conversion with Attenuation and Global Lepton Gradient
Masamichi Zaizen, Hiroki Nagakura

TL;DR
This study investigates how attenuation and global lepton gradients influence fast neutrino-flavor conversion in supernovae and neutron-star mergers, revealing conditions that suppress or promote flavor coherence.
Contribution
The paper introduces a global quantum kinetic simulation approach with an attenuated Hamiltonian and provides an approximate formula for adiabaticity relevant to astrophysical models.
Findings
Steep radial lepton gradients can suppress FFC.
Attenuation lengthens flavor growth timescales.
An approximate adiabaticity formula is provided for use in models.
Abstract
Fast neutrino-flavor conversion (FFC) can nontrivially alter neutrino radiation field in core-collapase supernovae (CCSN) and binary neutron-star merger (BNSM) remnants. However, its interplay with global geometry remains poorly understood because microscopic flavor conversion scales are much shorter than global transport scales. We perform global quantum kinetic neutrino transport simulations in spherical geometry with neutrino and matter backgrounds, using an attenuated oscillation Hamiltonian. We find that steep radial lepton gradients can suppress FFC, whereas the suppression is highly sensitive to the adopted attenuation parameter. This behavior is explained by an adiabatic condition: flavor coherence can grow sufficiently only while the flavor wave remains on the unstable branch in the local dispersion relation during propagation. Background variation shifts the unstable branch,…
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.
