We consider spherically symmetric higher-dimensional solutions of Einstein'
s equations with a bulk cosmological constant and n transverse dimensions.
In contrast to the case of one or two extra dimensions we find no solutions
that localize gravity when n greater than or equal to 3, for strictly loca
l topological defects. We discuss global topological defects that lead to t
he localization of gravity and estimate the corrections to Newton's law. We
show that the introduction of a bulk "hedgehog" magnetic field leads to a
regular geometry and localizes gravity on the 3-brane with either a positiv
e, zero or negative bulk cosmological constant. The corrections to Newton's
law on the 3-brane are parametrically the same as for the case of one tran
sverse dimension. (C) 2000 Elsevier Science B.V. All rights reserved.