PreprintarXiv licencearXiv
Neutrino Oscillations without Mass: A Re-analysis of KamLAND Data following the Dirac Equation in Curved Spacetime
Abstract
The Dirac equation in stationary curved spacetime implies that describing two-flavor neutrino oscillations requires treating the invariant mass and conserved energy of each propagating state distinctly, as gravity affects energy differently than mass. By re-analysing the publicly released KamLAND dataset, we show that modeling flavor states of massless neutrinos as two-level quantum states with energy-dependent level splitting, analogous to modified Jaynes-Cummings models, results in a higher-likelihood fit to the observed data than the standard massive-neutrino paradigm.
Related
- Neutrino oscillations inside ultrarelativistic matter: on the role of the Tolman VI spacetime
- Neutrino oscillations inside ultrarelativistic matter: on the role of the Tolman VI spacetime
- When can decoherence reveal a Majorana phase? A phase-covariance no-go theorem for two-flavor neutrino oscillations
- Quantum field-theoretical description of solar neutrino oscillations
- Atmospheric Neutrino Oscillations: the Full Picture
BibTeX
@misc{hossain2026neutrino,
title = {{Neutrino Oscillations without Mass: A Re-analysis of KamLAND Data following the Dirac Equation in Curved Spacetime}},
author = {Golam Mortuza Hossain and Pushpit Kumar},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.39638},
eprint = {2609.39638},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.39638},
}
RIS
TY - UNPB
TI - Neutrino Oscillations without Mass: A Re-analysis of KamLAND Data following the Dirac Equation in Curved Spacetime
AU - Golam Mortuza Hossain
AU - Pushpit Kumar
PY - 2026
DA - 2026/09/30
PB - arXiv
DO - 10.48550/arxiv.2609.39638
UR - https://arxiv.org/abs/2609.39638
AB - The Dirac equation in stationary curved spacetime implies that describing two-flavor neutrino oscillations requires treating the invariant mass and conserved energy of each propagating state distinctly, as gravity affects energy differently than mass. By re-analysing the publicly released KamLAND dataset, we show that modeling flavor states of massless neutrinos as two-level quantum states with energy-dependent level splitting, analogous to modified Jaynes-Cummings models, results in a higher-likelihood fit to the observed data than the standard massive-neutrino paradigm.
ER -