Effective Photon Mass Suppression by Path-Ensemble Averaging: A Phenomenological Hypothesis

We examine the phenomenological hypothesis that the photon effective mass entering macroscopic propagation is a suppressed value $\tilde{m}=m_{0}/N$ where $m_{0}$ is an experimental upper bound and $N$ a dimensionless suppression factor. We state explicitly that this relation is an ansatz: it is not derived from the standard path integral, and naive path-counting is mathematically ruled out. We compute the Compton length and the dispersion delay as functions of $N$ and show that, under model-dependent galactic bounds on the Proca vector-potential energy, the ansatz requires $N\ge3\times10^{8}-10^{9}$. The associated time-of-flight signature is many orders of magnitude below any foreseeable sensitivity, making the hypothesis consistent but currently unfalsifiable by dispersion tests. We outline how $N$ could rigorously emerge from the Euclidean partition function of a hidden sector with discrete $\mathbb{Z}_{N}$ symmetry or large-$N$ gauge dynamics.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-09-29
DOI
https://doi.org/10.5281/zenodo.23024947
Primary Topic
High-Energy Particle Collisions Research
Type
preprint
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preprint

Effective Photon Mass Suppression by Path-Ensemble Averaging: A Phenomenological Hypothesis

Jean-yves Lozac'h
Zenodo (CERN European Organization for Nuclear Research)
High-Energy Particle Collisions Research
preprint

Effective Photon Mass Suppression by Path-Ensemble Averaging: A Phenomenological Hypothesis

Jean-yves Lozac'h
preprint en

Abstract

We examine the phenomenological hypothesis that the photon effective mass entering macroscopic propagation is a suppressed value $\tilde{m}=m_{0}/N$ where $m_{0}$ is an experimental upper bound and $N$ a dimensionless suppression factor. We state explicitly that this relation is an ansatz: it is not derived from the standard path integral, and naive path-counting is mathematically ruled out. We compute the Compton length and the dispersion delay as functions of $N$ and show that, under model-dependent galactic bounds on the Proca vector-potential energy, the ansatz requires $N\ge3\times10^{8}-10^{9}$. The associated time-of-flight signature is many orders of magnitude below any foreseeable sensitivity, making the hypothesis consistent but currently unfalsifiable by dispersion tests. We outline how $N$ could rigorously emerge from the Euclidean partition function of a hidden sector with discrete $\mathbb{Z}_{N}$ symmetry or large-$N$ gauge dynamics.

Zenodo (CERN European Organization for Nuclear Research)
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