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We analyze the stability of the Einstein static universe by considering homogeneous scalar perturbations in the context of f(R) modified theories of gravity.
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W. Hu and I. Sawicki, “Models of f(R) Cosmic Acceleration that Evade Solar-System Tests,” 0705.1158 [astro-ph]
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I. Sawicki and W. Hu, “Stability of cosmological solution in f ( R ) f(R) models of gravity,” [astro-ph/0702278]
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L. Amendola and S. Tsujikawa, “Phantom crossing, equation-of-state singularities, and local gravity constraints in f ( R ) f(R) models,” 0705.0396 [astro-ph]
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S. Seahra, Private communication, (2007)
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M. Amarzguioui, O. Elgaroy, D. F. Mota and T. Multamaki, Astron. Astrophys. 454
2041
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