Recent results of Trudinger on isoperimetric inequalities for non-conv
ex bodies are applied to the gravitational collapse of a lightlike she
ll of matter to form a black hole. Using some integral identities for
co-dimension-two surfaces in Minkowski spacetime, the area A of the ap
parent horizon is shown to be bounded above in terms of the mass M by
16 pi G(2)M(2), which is consistent with the cosmic censorship hypothe
sis. The results hold in four spacetime dimensions and above.