Analytical solutions for Maxwell-scalar system on radially symmetric spacetimes
I. Andrade, D. Bazeia, M.A. Marques, R. Menezes, G.J. Olmo

TL;DR
This paper derives analytical solutions for Maxwell-scalar systems on radially symmetric spacetimes, exploring conditions for minimal energy configurations, stability, and mapping to kink solutions in lower dimensions.
Contribution
It introduces a formalism to find analytical solutions for Maxwell-scalar models on symmetric spacetimes and establishes their stability and energy properties.
Findings
Analytical solutions for specific spacetimes are obtained.
Energy density of solutions is finite.
Solutions obeying the first-order equations are stable.
Abstract
We investigate Maxwell-scalar models on radially symmetric spacetimes in which the gauge and scalar fields are coupled via the electric permittivity. We find the conditions that allow for the presence of minimum energy configurations. In this formalism, the charge density must be written exclusively in terms of the components of the metric tensor and the scalar field is governed by first-order equations. We also find a manner to map the aforementioned equation into the corresponding one associated to kinks in spacetime dimensions, so we get analytical solutions for three specific spacetimes. We then calculate the energy density and show that the energy is finite. The stability of the solutions against contractions and dilations, following Derrick's argument, and around small fluctuations in the fields is also investigated. In this direction, we show that the solutions obeying…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Gas Dynamics and Kinetic Theory · Black Holes and Theoretical Physics
