The time evolution of a large-amplitude bubble of a disoriented chiral cond
ensate (DCC) is studied. It is found that the evolution of such objects may
have a relatively long predecay stage. A simple explanation of such a dela
y is proposed for the case of the DCC hubble decay. This delay is associate
d with the existence of approximate multisoliton solutions to the relevant
radial sine-Gordon equation in (3+1) dimensions at a large hubble radius. (
C) 2001 MAIK "Nauka/Interperiodica".