Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory
Symmetry 2023, 15, 1970 We demonstrate that the Finite-Time-Path Field Theory is an adequate tool for calculating neutrino oscillations. We apply this theory using a mass-mixing Lagrangian which involves the correct Dirac spin and chirality structure and a Pontecorvo-Maki-Nakagawa-Sakata (PMNS)-like...
Saved in:
Main Authors: | , |
---|---|
Format: | Journal Article |
Language: | English |
Published: |
20-11-2023
|
Subjects: | |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Summary: | Symmetry 2023, 15, 1970 We demonstrate that the Finite-Time-Path Field Theory is an adequate tool for
calculating neutrino oscillations. We apply this theory using a mass-mixing
Lagrangian which involves the correct Dirac spin and chirality structure and a
Pontecorvo-Maki-Nakagawa-Sakata (PMNS)-like mixing matrix. The model is exactly
solvable. The Dyson-Schwinger equations transform propagators of the input free
(massless) flavor neutrinos into a linear combination of oscillating (massive)
neutrinos. The results are consistent with the predictions of the PMNS matrix
while allowing for extrapolation to early times. |
---|---|
Bibliography: | ZTF-EP-23-04 and RBI-ThPhys-2023-27 |
DOI: | 10.48550/arxiv.2311.11875 |