Inflation driven by non-linear electrodynamics

We investigate the inflation driven by a nonlinear electromagnetic field based on an NLED lagrangian density L-nled = -Ff (F), where f (F) is a general function depending on F. We first formulate an f-NLED cosmological model with a more general function f (F) and show that all NLED models can be expressed in this framework; then, we investigate in detail two interesting examples of the function f (F). We present our phenomenological model based on a new Lagrangian for NLED. Solutions to the field equa-tions with the physical properties of the cosmological param-eters are obtained. We show that the early Universe had no Big-Bang singularity, which accelerated in the past. We also investigate the qualitative implications of NLED by study -ing the inflationary parameters, like the slow-roll parameters, spectral index n(s), and tensor-to-scalar ratio r, and compare our results with observational data. Detailed phase-space analysis of our NLED cosmological model is performed with and without matter source. As a first approach, we consider the motion of a particle of unit mass in an effective potential. Our systems correspond to fast-slow systems for physical values of the electromagnetic field and the energy densities at the end of inflation. We analyze a complementary system using Hubble-normalized variables to investigate the cosmo-logical evolution before the matter-dominated Universe.

Automated summary

This study investigates inflation driven by a nonlinear electromagnetic field based on an NLED lagrangian density. The study formulates an f-NLED cosmological model with a general function f (F) and explores two interesting examples of the function f (F). The study also analyzes the implications of NLED by studying inflationary parameters and compares the results with observational data.