  This work investigates the spherically symmetric thin-shell wormhole
solutions in four-dimensional Einstein-Gauss-Bonnet theory and explores their
stabilities under radial, linear perturbations. These solutions are typically
traversable and characterized by a thin-shell throat in accordance with
Israel's junction conditions. In asymptotically flat and AdS spacetimes with a
negative Gauss-Bonnet coupling constant, stable neutral wormholes are
encountered when the magnitude of the coupling constant becomes significant.
The throats of such wormholes are sustained by ordinary matter and possess
finite radii. In asymptotically dS spacetimes, no stable neutral wormhole
featuring ordinary matter is observed. On the other hand, for positive
Gauss-Bonnet coupling constant, stable thin-shell wormhole solutions can be
established when the throats are exclusively supported by exotic matter.
Moreover, stable charged wormholes comprised of ordinary matter are found
universally in the asymptotically flat, AdS, and dS spacetimes. Unlike their
neutral counterparts, the throat radii of such charged wormholes can be
arbitrarily small. However, as the charge becomes more significant, such
solutions only remain stable when supported by exotic matter.
