Accounting for the Heisenberg and Pauli principles in the kinetic approach to neutrino oscillations
A. Kartavtsev

TL;DR
This paper demonstrates that the kinetic approach to neutrino oscillations, when initialized with quantum-consistent conditions, inherently accounts for quantum principles like the Heisenberg and Pauli principles, impacting supernova neutrino phenomenology.
Contribution
It establishes the equivalence of quantum-mechanical and kinetic approaches for collisionless neutrinos and shows how quantum principles are incorporated through initial conditions.
Findings
Kinetic and quantum approaches are equivalent in collisionless limit.
Initial conditions can encode quantum principles like uncertainty and Pauli exclusion.
Wave packet separation affects supernova neutrino behavior.
Abstract
While oscillations of solar neutrinos are usually studied using the single-particle quantum-mechanical approach, flavor conversions of supernovae neutrinos are typically analyzed using the kinetic equation for the matrix of densities due to the necessity of including also the scattering processes. Using the Wigner formulation of quantum mechanics we show the equivalence of the quantum-mechanical and kinetic approaches in the limit of collisionless neutrino propagation (in a background medium). Based on this observation we also argue that solutions of the kinetic equation account for the Heisenberg uncertainty principle and the related effect of wave packet separation (for single neutrinos), as well as the Pauli exclusion principle, if the initial conditions are consistent with these fundamental quantum principles. Such initial conditions can be constructed e.g. by identifying the matrix…
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