We study the head-on collision of black holes starting from unsymmetrized,
Brill-Lindquist type data for black holes with non-vanishing initial linear
momentum. Evolution of the initial data is carried out with the "close lim
it approximation," in which small initial separation and momentum are assum
ed, and second-order perturbation theory is used. We find agreement that is
remarkably good, and that in some ways improves with increasing momentum.
This work extends a previous study in which second order perturbation calcu
lations were used for momentarily stationary initial data, and another stud
y in which linearized perturbation theory was used for initially moving hol
es. In addition to supplying answers about the collisions, the present work
has revealed several subtle points about the use of higher order perturbat
ion theory, points that did not arise in the previous studies. These points
include issues of normalization, and of comparison with numerical simulati
ons, and will be important to subsequent applications of approximation meth
ods for collisions. [S0556-2821(98)03822-3].