Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2002-03-22
Phys.Rev. D65 (2002) 104035
Physics
High Energy Physics
High Energy Physics - Theory
9 pages, RevTex, to appear in Phys. Rev. D
Scientific paper
10.1103/PhysRevD.65.104035
After reviewing the main characteristics of the spacetime of accelerating universes driven by a quintessence scalar field with constant equation of state $\omega$, we investigate in this paper the classical stability of such spaces to cosmological perturbations, particularizing in the case of a closed geometry and equation of state $\omega=-2/3$. We conclude that this space is classically stable and conjecture that accelerating universes driven by quintessential fields have "no-hair".
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