Electrostatic spherically symmetric configurations in gravitating nonlinear electrodynamics
J. Diaz-Alonso, D. Rubiera-Garcia

TL;DR
This paper analyzes gravitating electrostatic spherically symmetric solutions in nonlinear electrodynamics coupled to gravity, revealing how their structure depends on flat space solutions and identifying new features for finite-energy solitons.
Contribution
It characterizes the structure of G-ESS solutions in admissible nonlinear electrodynamics models, linking them to flat space behaviors and exploring new qualitative features for finite-energy solitons.
Findings
G-ESS solutions are determined by flat space asymptotics.
Divergent-energy solutions resemble Reissner-Nordström structure.
Finite-energy solutions exhibit new qualitative features related to mass, charge, and energy.
Abstract
We perform a study of the gravitating electrostatic spherically symmetric (G-ESS) solutions of Einstein field equations minimally coupled to generalized non-linear abelian gauge models in three space dimensions. These models are defined by lagrangian densities which are general functions of the gauge field invariants, restricted by some physical conditions of admissibility. They include the class of non-linear electrodynamics supporting ESS non-topological soliton solutions in absence of gravity. We establish that the qualitative structure of the G-ESS solutions of admissible models is fully characterized by the asymptotic and central-field behaviours of their ESS solutions in flat space (or, equivalently, by the behaviour of the lagrangian densities in vacuum and on the point of the boundary of their domain of definition, where the second gauge invariant vanishes). The structure of…
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