Circularly symmetric thin-shell wormholes in F(R) gravity with (2+1)-dimensions
Cecilia Bejarano, Ernesto F. Eiroa, Griselda Figueroa-Aguirre

TL;DR
This paper constructs and analyzes the stability of circularly symmetric thin-shell wormholes in (2+1)-dimensional F(R) gravity with constant scalar curvature, demonstrating stable configurations with normal matter under certain conditions.
Contribution
It introduces a new class of thin-shell wormholes in (2+1)-dimensional F(R) gravity and examines their stability, which was not previously explored in this context.
Findings
Stable wormhole configurations with normal matter are possible.
Asymptotically anti-de Sitter charged wormholes can be stable.
Stability depends on specific parameter ranges.
Abstract
Within the framework of theories of gravity with (2+1)-dimensions and constant scalar curvature , we construct a family of thin-shell wormholes with circular symmetry and we analyze the stability of the static configurations under radial perturbations. We show an example of asymptotically anti-de Sitter thin-shell wormholes with charge, finding that stable configurations with normal matter are possible for a suitable range of the parameters.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Geophysics and Gravity Measurements
