  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.
$V^{\prime \prime}\left(a_{0}\right) >0$. This may serve as the master equation
in all stability problems for the cylindrical thin-shell wormholes.
