  We discuss the graviton absorption probability (greybody factor) and the
cross-section of a higher-dimensional Schwarzschild black hole (BH). We are
motivated by the suggestion that a great many BHs may be produced at the LHC
and bearing this fact in mind, for simplicity, we shall investigate the
intermediate energy regime for a static Schwarzschild BH. That is, for
$(2M)^{1/(n-1)}\omega\sim 1$, where $M$ is the mass of the black hole and
$\omega$ is the energy of the emitted gravitons in $(2+n)$-dimensions. To find
easily tractable solutions we work in the limit $l \gg 1$, where $l$ is the
angular momentum quantum number of the graviton.
