On the electromagnetic nature of dark energy and the origin of cosmic magnetic fields
Jose Beltran Jimenez, Antonio L. Maroto

TL;DR
This paper proposes that quantum electromagnetic fields in an expanding universe can explain dark energy and cosmic magnetic fields without new physics, linking inflationary fluctuations to observed phenomena.
Contribution
It introduces an extended electromagnetic theory allowing a propagating scalar state, which can be excited gravitationally and explains dark energy and magnetic field generation.
Findings
Primordial quantum fluctuations produce electromagnetic modes acting as a cosmological constant.
The theory aligns with local gravity tests and avoids instabilities.
Magnetic fields >10^{-12} G with large coherence lengths can be generated.
Abstract
In this work we consider quantum electromagnetic fields in an expanding universe. We start by reviewing the difficulties found when trying to impose the Lorenz condition in a time-dependent geometry. Motivated by this fact, we explore the possibility of extending the electromagnetic theory by allowing the scalar state which is usually eliminated by means of the Lorenz condition to propagate, preserving at the same time the dynamics of ordinary transverse photons. We show that the new state cannot be generated by charged currents, but it breaks conformal invariance and can be excited gravitationally. In fact, primordial quantum fluctuations produced during inflation can give rise to super-Hubble temporal electromagnetic modes whose energy density behaves as a cosmological constant. The value of the effective cosmological constant is shown to agree with observations provided inflation…
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