Stable thin-shell wormholes with a Chaplygin gas in Einstein-Maxwell-Gauss-Bonnet gravity

TL;DR

This paper investigates the stability of thin-shell wormholes within Einstein-Maxwell-Gauss-Bonnet gravity, analyzing various equations of state including generalized Chaplygin gas and its effects on stability in five dimensions.

Contribution

It introduces a generalized framework for analyzing thin-shell wormhole stability with arbitrary equations of state in higher-dimensional gravity.

Findings

GB parameter influences wormhole stability

Generalized Chaplygin gas affects stability conditions

Numerical analysis in 5D confirms theoretical predictions

Abstract

We study the stability of thin-shell wormholes in Einstein-Maxwell-Gauss-Bonnet gravity. The equation of state of the thin shell wormhole is considered first to obey a generalized Chaplygin gas and then we generalize it to an arbitrary state function which covers all known cases studied so far. In particular we study the modified Chaplygin gas and give an assessment for a general parotropic fluid. Our study is in d-dimensions and with numerical analysis in d=5 we show the effect of the GB parameter in the stability of thin-shell wormholes against the radial perturbations.