  In general relativity one of the most fundamental issues consists in defining
a generally acceptable definition for the energy-momentum density. As a
consequence, many coordinate-dependent definitions have been presented, whereby
some of them utilize appropriate energy-momentum complexes. We investigate the
energy-momentum distribution for a metric exterior to a spherically symmetric
black hole in the brane world by applying the Landau-Lifshitz and Weinberg
prescriptions. In both the aforesaid prescriptions, the energy thus obtained
depends on the radial coordinate, the mass of the black hole and a parameter
$\lambda_{0}$, while all the momenta are found to be zero. It is shown that for
a special value of the parameter $\lambda_{0}$, the Schwarzschild space-time
geometry is recovered. Some particular and limiting cases are also discussed.
