  In this second paper in our series, we continue to test primordial scenarios
of globular cluster formation which predict that globular clusters formed in
the early universe in the potential of dark matter minihalos. In this paper we
use high-resolution N-body simulations to model tidal stripping experienced by
primordial dark-matter dominated globular clusters in the static gravitational
potential of the host dwarf galaxy. We test both cuspy Navarro-Frenk-White
(NFW) and flat-core Burkert models of dark matter halos. Our primordial
globular cluster with an NFW dark matter halo survives severe tidal stripping,
and after 10 orbits is still dominated by dark matter in its outskirts. Our
cluster with Burkert dark matter halo loses almost all its dark matter to tidal
stripping, and starts losing stars at the end of our simulations. The results
of this paper reinforce our conclusion in Paper I that current observations of
globular clusters are consistent with the primordial picture of globular
cluster formation.
