We numerically study classical time evolutions of Kaluza-Klein bubble space
-time which has negative energy after a decay of vacuum. As the zero-energy
Witten bubble space-time, where the bubble expands infinitely, the subsequ
ent evolutions of the Brill-Horowitz momentarily static initial data show t
hat the bubble will expand in terms of the area. At first glance, this resu
lt may support the Corley-Jacobson conjecture that the bubble will expand f
orever as well as Witten's bubble. The irregular signatures, however, can b
e seen in the behavior of the lapse function in the maximal slicing gauge a
nd the divergence of the Kretchman invariant. Since there is no appearance
of the apparent horizon, we suspect the appearance of a naked singularity a
s the final fate of this space-time.