A class of grand unified theories with symmetry breaking scale of orde
r 10(16) GeV have a Hi,ags particle with mass in the TeV scale. The co
smology of such theories is very different from usual. We study the co
smic strings obtained in such theories. These strings are much fatter
than usual and their mass per unit length is reduced, resulting in a s
ignificant reduction in their cosmological effects. We also study the
temperature evolution of such models. (C) 1998 Elsevier Science B.V. A
ll rights reserved.