We study the onset of Goldstone phenomenon in a hybrid inflation scenario.
The physically motivated range of parameters is analyzed in order to meet the
cosmological constraints. Classical equations of motion are solved and the
evolution through the spontaneous symmetry breaking is followed. We emphasize
the role of topological defects that partially maintain the disordered phase
well after the waterfall. We study the emergence of the Goldstone excitations
and their role in the onset of the radiation dominated universe.Comment: 10 pages with 7 figures. Contribution to Strong and Electroweak
Matter (Heidelberg, 2002