We investigate collisions between two spherical massive shells in vacuum sp
ace-time by assuming that the shells are transparent. We give an expression
for the energy transfer and the change in the 3-momentum due to the collis
ion. Compared with the Newtonian situation, the relativistic effect always
increases the energy transfer. In particular, in a collision close to the s
ingularity and the horizon defined in the region between the shells, the en
ergy transfer can be arbitrarily large. However, in such cases, the collisi
on is not observable for the asymptotic observer. Further, we discuss a sit
uation similar to the shell crossing on a spherical void wall of the horizo
n scale. In this case, for some parameter choices, the outer shell initiall
y going outward may suddenly change its motion to contraction due to a rela
tivistic effect when it crosses with the inner shell.