Coherence of oscillations in matter and supernova neutrinos
Yago P. Porto-Silva, Alexei Yu. Smirnov

TL;DR
This paper investigates neutrino oscillation coherence in matter with varying density profiles, revealing energy-dependent coherence lengths, infinite coherence conditions, and implications for supernova neutrino observations.
Contribution
It introduces the concept of energy ranges with infinite coherence in matter and analyzes their effects on neutrino oscillations in supernova environments.
Findings
Existence of energy ranges with infinite coherence in matter.
Coherence length dependence on neutrino energy and density profiles.
Implications for supernova neutrino flavor transformations.
Abstract
We study the propagation coherence for neutrino oscillations in media with different density profiles. For each profile, we find the dependence of the coherence length, , on neutrino energy and address the issue of correspondence of results in the distance and energy-momentum representations. The key new feature in matter is existence of energy ranges with enhanced coherence around the energies of "infinite coherence" at which . In the configuration space, the infinite coherence corresponds to equality of the (effective) group velocities of the eigenstates. In constant density medium, there is a unique , which coincides with the MSW resonance energy of oscillations of mass states and is close to the MSW resonance energy of flavor states. In the case of massless neutrinos or negligible masses in a very dense medium the coherence persists…
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