Early dark energy induced by non-linear electrodynamics
H. B. Benaoum, Luz \'Angela Garc\'ia, Leonardo Casta\~neda

TL;DR
This paper proposes a model of early dark energy driven by non-linear electrodynamics, which can alleviate the Hubble and sigma_8 tensions by predicting an earlier universe structure formation and a shorter age.
Contribution
It introduces a novel parametrization linking early dark energy to non-linear electrodynamics, fitting observational data and addressing key cosmological tensions.
Findings
Predicts an earlier formation of cosmic structures.
Alleviates the Hubble and sigma_8 tensions.
Provides best-fit parameters consistent with multiple datasets.
Abstract
In this work, we introduce a parametrization of early dark energy that mimics radiation at early times and governs the present acceleration of the Universe. We show that such parametrization models non-linear electrodynamics in the early Universe and investigate the cosmological viability of the model. In our scenario, the early dark energy is encoded in the non-linearity of the electromagnetic fields through a parameter that changes the Lagrangian of the system, and the parameters and , that define the departure from the standard model constant equation of state. We use a Bayesian method and the modular software \textsc{CosmoSIS} to find the best values for the model's free parameters with precomputed likelihoods from Planck 2018, primordial nucleosynthesis data, inferred distances from different wide galaxy surveys and luminosity distances of SNIa from…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Radio Astronomy Observations and Technology
