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We revisit the stability analysis of cylindrical thin-shell wormholes which have been studied in literature so far. Our approach is more systematic and in parallel to the method which is used in spherically symmetric thin-shell wormholes. The stability condition is summarized as the positivity of the second derivative of an effective potential at the equilibrium radius, i.e., V^''(a₀)>0. This may serve as the master equation in all stability problems for the cylindrical thin-shell wormholes.
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Mazharimousavi et al. (2014) studied this question.
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