Thin-shell wormholes in Einstein-Born-Infeld theory
Ernesto F. Eiroa, Griselda Figueroa-Aguirre
TL;DR
This paper constructs and analyzes the stability of spherically symmetric thin-shell wormholes within Einstein-Born-Infeld theory, using a generalized Chaplygin gas at the throat to explore their physical viability.
Contribution
It introduces a novel approach by combining Born-Infeld electrodynamics with Einstein gravity to model thin-shell wormholes with a Chaplygin gas, and assesses their stability.
Findings
Wormholes constructed are stable under certain conditions.
The generalized Chaplygin gas influences the stability criteria.
The model extends previous work by incorporating nonlinear electrodynamics.
Abstract
We construct spherically symmetric thin-shell wormholes with a generalized Chaplygin gas at the throat, in Born-Infeld electrodynamics coupled to Einstein gravity. We analyze their stability under radial perturbations.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics