  Dark matter halos are common in galaxies and globular clusters, making it
possible to use dark matter density profiles to construct transverse wormholes.
In reference [1], an approximate solution of the traversable wormhole
satisfying the isotropic pressure condition is constructed by using the dark
matter density profile. However, approximate solutions limit the discussion of
traversable wormholes to a large extent. In this work, we construct the exact
solution of the traversable wormhole in the case of rotation in the dark matter
halo. We have written analytical expressions for the Kerr-like traversable
wormhole metric for the dark matter density profile in galaxies corresponding
to different dark matter models, respectively. These rotating traversable
wormholes are jointly determined by the dark matter characteristic density and
the scale radius. At the same time, we have also analyzed the energy conditions
satisfied by these rotationally traversable wormholes.
