  With the aim of studying rotating quark-gluon plasma (QGP), holographically,
from a top-down approach, the study of the effect of rotation on the
deconfinement temperature of thermal QCD-like theories at intermediate coupling
from ${\cal M}$-theory was missing in the literature. This paper fills this
gap. The gravity dual includes a rotating cylindrical black hole. In the
presence of rotation, from a semi-classical computation, we found that the
deconfinement temperature is inversely proportional to the Lorentz factor,
which suggests that the deconfinement temperature decreases with the increase
of rotation. Further, we found that in the small angular velocity limit,
results from higher derivative correction at ${\cal O}(R^4)$ do not change and
are the same as in arXiv:2108.05372. The "UV-IR mixing", "Flavor Memory"
effect, and "non-renormalization of $T_c$" in the ${\cal M}$-theory dual are
similar to the ones observed in arXiv:2108.05372.
