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

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