de Broglie-Proca and Bopp-Podolsky massive photon gases in cosmology
R.R. Cuzinatto, E.M. de Morais, L.G. Medeiros, C. Naldoni de Souza,, B.M. Pimentel

TL;DR
This paper explores how massive photons, modeled by de Broglie-Proca and Bopp-Podolsky theories, influence cosmic evolution, finding that photon mass has negligible effect on the universe's expansion rate.
Contribution
It provides the first detailed analysis of the impact of massive photon gases on cosmological dynamics using two generalized electrodynamics models.
Findings
Photon mass does not significantly change the scale factor evolution.
The equation of state for massive photons is derived from dispersion relations.
Results are consistent with the massless photon case for extreme photon masses.
Abstract
We investigate the influence of massive photons on the evolution of the expanding universe. Two particular models for generalized electrodynamics are considered, namely de Broglie-Proca and Bopp-Podolsky electrodynamics. We obtain the equation of state (EOS) for each case using dispersion relations derived from both theories. The EOS are inputted into the Friedmann equations of a homogeneous and isotropic space-time to determine the cosmic scale factor . It is shown that the photon non-null mass does not significantly alter the result valid for a massless photon gas; this is true either in de Broglie-Proca's case (where the photon mass is extremely small) or in Bopp-Podolsky theory (for which is extremely large).
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