  When the Planck scale is as low as TeV scale, there will be chances to
produce Black holes (BH's) at future colliders. Generally, BH's produced via
pariticle collisions could have non-zero angular momentum. We estimate the
production cross section of spinning and non-spinning BH's for future
colliders. Although the production cross section for the rotating BH is much
suppressed by angular momentum dependent factor, the total cross section could
be $\sim 2 -3$ times enhanced for the case of $\delta =4-6$.
