Stable accelerating universe with no hair
Pedro F. Gonzalez-Diaz (IMAFF, CSIC, Madrid)

TL;DR
This paper examines the classical stability of accelerating universes driven by quintessence fields, specifically in closed geometries with a constant equation of state, and suggests they have a 'no-hair' property.
Contribution
It demonstrates the classical stability of closed accelerating universes with a specific quintessence equation of state and introduces the 'no-hair' conjecture for such cosmological models.
Findings
Closed universe with ω=-2/3 is classically stable.
Accelerating universes driven by quintessence are conjectured to have 'no-hair'.
Provides stability analysis for specific cosmological conditions.
Abstract
After reviewing the main characteristics of the spacetime of accelerating universes driven by a quintessence scalar field with constant equation of state , 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 . We conclude that this space is classically stable and conjecture that accelerating universes driven by quintessential fields have "no-hair".
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