Abstract:
We have studied semiclassical models with a classical scalar field, giving exact solutions in the cases of a λ φ4 and an exponential self-interaction potential, in the last case we have also studied the influence of the vacuum polarization terms on the stability of the power-law solutions. We have also found cosmological exact solutions to the higher order gravitational equations derived from a Lagrangian with a R □k R structure, and investigated the stability of the de Sitter and Minkowski space-time in the sixth order approximation of this theory. ‡ Supported by scholarship of the Universidad de Buenos Aires.
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Citas:
---------- APA ----------
Chimento, L.P. & Zuccalá, N.A.
(2000)
. Cosmological models in semi-classical and higher order gravitational theories. Astrophysics and Space Science, 274(4), 837-849.
http://dx.doi.org/10.1023/A:1026574105476---------- CHICAGO ----------
Chimento, L.P., Zuccalá, N.A.
"Cosmological models in semi-classical and higher order gravitational theories"
. Astrophysics and Space Science 274, no. 4
(2000) : 837-849.
http://dx.doi.org/10.1023/A:1026574105476---------- MLA ----------
Chimento, L.P., Zuccalá, N.A.
"Cosmological models in semi-classical and higher order gravitational theories"
. Astrophysics and Space Science, vol. 274, no. 4, 2000, pp. 837-849.
http://dx.doi.org/10.1023/A:1026574105476---------- VANCOUVER ----------
Chimento, L.P., Zuccalá, N.A. Cosmological models in semi-classical and higher order gravitational theories. Astrophys. Space Sci. 2000;274(4):837-849.
http://dx.doi.org/10.1023/A:1026574105476