  In this work, we study the thin-shell wormholes in dRGT massive gravity. In
order to joint two bulks of the spacetime geometry, we first derive junction
conditions of the dRGT spacetime. This results the dynamics of the spherical
thin-shell wormholes in the dRGT theory. We show that the massive graviton
correction term of the dRGT theory in the Einstein equation is represented in
terms of the effective anisotropic pressure fluid. However, if there is only
this correction term, without invoking exotic fluids, we find that the
thin-shell wormholes can not be stabilized. We then examine the stability
conditions of the wormholes by introducing four existing models of the exotic
fluids at the throat. In addition, we analyze the energy conditions for the
thin-shell wormholes in the dRGT massive gravity by checking the null, weak,
and strong conditions at the wormhole throat. We show that in general the
classical energy conditions are violated by introducing all existing models of
the exotic fluids. Moreover, we quantify the wormhole geometry by using the
embedding diagrams to represent a thin-shell wormhole in the dRGT massive
gravity.
