Abstract:
Several isotropic, homogeneous cosmological models containing a self-interacting minimally coupled scalar field, a perfect fluid source and cosmological constant are solved. New exact, asymptotically stable solutions with an inflationary regime or a final Friedmann stage are found for some simple, interesting potentials. It is shown that the fluid and the curvature may determine how these models evolve for large times.
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Citas:
---------- APA ----------
Chimento, L.P. & Jakubi, A.S.
(1996)
. Scalar field cosmologies with perfect fluid in Robertson-Walker metric. International Journal of Modern Physics D, 5(1), 71-84.
http://dx.doi.org/10.1142/S0218271896000084---------- CHICAGO ----------
Chimento, L.P., Jakubi, A.S.
"Scalar field cosmologies with perfect fluid in Robertson-Walker metric"
. International Journal of Modern Physics D 5, no. 1
(1996) : 71-84.
http://dx.doi.org/10.1142/S0218271896000084---------- MLA ----------
Chimento, L.P., Jakubi, A.S.
"Scalar field cosmologies with perfect fluid in Robertson-Walker metric"
. International Journal of Modern Physics D, vol. 5, no. 1, 1996, pp. 71-84.
http://dx.doi.org/10.1142/S0218271896000084---------- VANCOUVER ----------
Chimento, L.P., Jakubi, A.S. Scalar field cosmologies with perfect fluid in Robertson-Walker metric. Int. J. Mod. Phys. D. 1996;5(1):71-84.
http://dx.doi.org/10.1142/S0218271896000084