Abstract:
In this paper the second Lyapunov method is used to study the stability of the de Sitter phase of cosmic expansion when the source of the gravitational field is a viscous fluid. Different inflationary scenarios related to reheating and decay of mini-black holes into radiation are investigated using an effective fluid described by time-varying thermodynamical quantities.
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Citas:
---------- APA ----------
Chimento, L.P., Jakubi, A.S. & Pavón, D.
(1999)
. Stability of inflationary solutions driven by a changing dissipative fluid. Classical and Quantum Gravity, 16(5), 1625-1635.
http://dx.doi.org/10.1088/0264-9381/16/5/312---------- CHICAGO ----------
Chimento, L.P., Jakubi, A.S., Pavón, D.
"Stability of inflationary solutions driven by a changing dissipative fluid"
. Classical and Quantum Gravity 16, no. 5
(1999) : 1625-1635.
http://dx.doi.org/10.1088/0264-9381/16/5/312---------- MLA ----------
Chimento, L.P., Jakubi, A.S., Pavón, D.
"Stability of inflationary solutions driven by a changing dissipative fluid"
. Classical and Quantum Gravity, vol. 16, no. 5, 1999, pp. 1625-1635.
http://dx.doi.org/10.1088/0264-9381/16/5/312---------- VANCOUVER ----------
Chimento, L.P., Jakubi, A.S., Pavón, D. Stability of inflationary solutions driven by a changing dissipative fluid. Classical Quantum Gravity. 1999;16(5):1625-1635.
http://dx.doi.org/10.1088/0264-9381/16/5/312