Abstract:
We investigate the simplest quintessence dissipative dark matter attractor cosmology characterized by a constant quintessence baryotropic index and a power-law expansion. We show a class of accelerated coincidence-solving attractor solutions converging to this asymptotic behavior. Despite its simplicity, such a "superattractor" regime provides a model of the recent universe that also exhibits an excellent fit to supernovae luminosity observations and no age conflict. Our best fit gives a= 1.71 ±0.29 for the power-law exponent. We calculate for this regime the evolution of density and entropy perturbations. ©2001 The American Physical Society.
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Citas:
---------- APA ----------
Chimento, L.P., Jakubi, A.S. & Zuccalâ, N.A.
(2001)
. Quintessence dissipative superattractor cosmology. Physical Review D, 63(10).
http://dx.doi.org/10.1103/PhysRevD.63.103508---------- CHICAGO ----------
Chimento, L.P., Jakubi, A.S., Zuccalâ, N.A.
"Quintessence dissipative superattractor cosmology"
. Physical Review D 63, no. 10
(2001).
http://dx.doi.org/10.1103/PhysRevD.63.103508---------- MLA ----------
Chimento, L.P., Jakubi, A.S., Zuccalâ, N.A.
"Quintessence dissipative superattractor cosmology"
. Physical Review D, vol. 63, no. 10, 2001.
http://dx.doi.org/10.1103/PhysRevD.63.103508---------- VANCOUVER ----------
Chimento, L.P., Jakubi, A.S., Zuccalâ, N.A. Quintessence dissipative superattractor cosmology. 2001;63(10).
http://dx.doi.org/10.1103/PhysRevD.63.103508