Cosmological solutions of a toy homogeneous isotropic universe filled with
a superfluid Bose condensate described by a complex scalar field (with rela
tivistic barotropic fluid interpretation) are studied. The eigenvalues of t
he tangent map for the resulting Hamiltonian system are used to classify th
e phase space regions and to understand the typical toy-universe evolution.
After a transient, inflation is obtained in the hyperbolic (real eigenvalu
es) region. This new independent eigenvalue-based inflationary criterion is
shown to be compatible and complementary to the standard slow roll-over co
nditions. For the later evolution of the toy-universe, a family of adiabati
c trajectories oscillating about a conventional cosmology filled with a rel
ativistic fluid is obtained once the system falls into the elliptic (imagin
ary eigenvalue) regions. The corresponding thermodynamic functions are comp
uted. (C) 2000 Elsevier Science B.V. All rights reserved.