Modified gravity and the stability of de Sitter space
arXiv:gr-qc/0509008 · doi:10.1103/PhysRevD.72.061501
Abstract
Within the context of modified gravity and dark energy scenarios of the accelerating universe, we study the stability of de Sitter space with respect to inhomogeneous perturbations using a gauge-independent formalism. In modified gravity the stability condition is exactly the same that one obtains from a homogeneous perturbation analysis, while the stability condition in scalar-tensor gravity is more restrictive.
5 pages, no figures, RevTeX, to appear in Phys. Rev. D (Rapid Communications section)
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