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This paper is devoted to the study of the stability of thin-shell wormholes from Kerr black hole. We employ Israel thin-shell formalism to evaluate surface stresses and study the behavior of energy conditions. The linearized stability of rotating thin-shell wormholes is analyzed by taking two different candidates of dark energy as exotic matter at thin-shell. It is found that generalized phantom model (Formula: see text which reduces to phantom equation of state as Formula: see text and Formula: see text, where Formula: see text is wormhole throat radius and Formula: see text is the proper time) yields more stable wormhole solutions as compared to the barotropic equation of state (Formula: see text, Formula: see text is the equation of state parameter and Formula: see text is the surface density) for particular ranges of equilibrium throat radius and the whole range of Formula: see text.
Sharif et al. (Thu,) studied this question.
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