arXiv · 2311.11875
Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory
Abstract
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.
Explore related subjects
Keep this discovery
Ivan Dadić, Dubravko Klabučar. 2023-11-20. Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory. https://doi.org/10.3390/sym15111970
Cite the original work for its findings. Save a collection to share your selection of sources.