  Exploiting the five-dimensional Schwarzschild black hole, we study the
geometrical natures of the higher dimensional black hole to yield the (6+1)
dimensional global embedding Minkowski space structure. We next obtain the
Hawking temperature on this five-dimensional manifold, whose result is
different from the four-dimensional one. On the contrary, the radial component
of the Einstein equation for the massive particles or photons on the
five-dimensional spacetime is shown to have the same form as the
four-dimensional black hole one. Moreover, we construct the effective potential
on equatorial plane of the restricted three-brane to investigate the behavior
of the particles or photons on this restricted brane.
