Lower Neutrino Mass Bound from SN1987A Data and Quantum Geometry
G. Lambiase, G. Papini, R. Punzi, G. Scarpetta

TL;DR
This paper establishes a lower bound on neutrino mass using a quantum geometric model and SN1987A neutrino data, aligning with existing upper bounds, and also derives constraints on intergalactic electron density.
Contribution
It introduces a geometrical quantum mechanics framework to derive neutrino mass bounds from astrophysical data and applies it to photons to estimate intergalactic electron density.
Findings
Neutrino mass lower bound: $m_ u \,\gtrsim 10^{-4}-10^{-3}$ eV
Neutrino mass bounds agree with current upper limits
Lower limit on intergalactic electron density consistent with baryon measurements
Abstract
A lower bound on the light neutrino mass is derived in the framework of a geometrical interpretation of quantum mechanics. Using this model and the time of flight delay data for neutrinos coming from SN1987A, we find that the neutrino masses are bounded from below by eV, in agreement with the upper bound eV currently available. When the model is applied to photons with effective mass, we obtain a lower limit on the electron density in intergalactic space that is compatible with recent baryon density measurements.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
