Do consistent $F(R)$ models mimic General Relativity plus $\Lambda$?

[1]  I. Sawicki,et al.  Stability of cosmological solutions in f ( R ) models of gravity , 2007, astro-ph/0702278.

[2]  L. Amendola,et al.  Conditions for the cosmological viability of f(R) dark energy models , 2006, gr-qc/0612180.

[3]  T. Sotiriou Curvature scalar instability in f(R) gravity , 2006, gr-qc/0611107.

[4]  M. Trodden,et al.  Dynamics of Linear Perturbations in f(R) Gravity , 2006, astro-ph/0611321.

[5]  I. Sawicki,et al.  Large scale structure of f(R) gravity , 2006, astro-ph/0610532.

[6]  C. V. D. Bruck,et al.  Viability of f(R) theories with additional powers of curvature , 2006, hep-th/0608015.

[7]  S. Nojiri,et al.  MODIFIED F (R) GRAVITY CONSISTENT WITH REALISTIC COSMOLOGY: FROM A MATTER DOMINATED EPOCH TO A DARK ENERGY UNIVERSE , 2006, hep-th/0608008.

[8]  A. Dobado,et al.  f ( R ) gravity without a cosmological constant , 2006, gr-qc/0607118.

[9]  V. Faraoni Solar system experiments do not yet veto modified gravity models , 2006, gr-qc/0607016.

[10]  S. Capozziello,et al.  Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase , 2006, astro-ph/0604431.

[11]  M. Trodden,et al.  Ghosts, instabilities, and superluminal propagation in modified gravity models , 2006, astro-ph/0604154.

[12]  L. Amendola,et al.  Are f(R) dark energy models cosmologically viable? , 2006, Physical review letters.

[13]  V. Faraoni,et al.  Stability of modified gravity models , 2005, gr-qc/0511094.

[14]  Alvaro Núñez,et al.  Ghost constraints on modified gravity , 2004, hep-th/0411102.

[15]  S. Carroll,et al.  Cosmology of generalized modified gravity models , 2004, Physical Review D.

[16]  D. Vollick COMMENT: On the viability of the Palatini form of 1/R gravity , 2003, gr-qc/0312041.

[17]  S. Nojiri,et al.  Modified Gravity with ln R Terms and Cosmic Acceleration , 2003, hep-th/0308176.

[18]  E. Flanagan Palatini form of 1/R gravity. , 2003, Physical review letters.

[19]  S. Nojiri,et al.  Modified gravity with negative and positive powers of the curvature: Unification of the inflation and of the cosmic acceleration , 2003, hep-th/0307288.

[20]  T. Chiba 1/R gravity and scalar-tensor gravity , 2003, astro-ph/0307338.

[21]  A. Dolgov,et al.  Can modified gravity explain accelerated cosmic expansion , 2003, astro-ph/0307285.

[22]  R. Dick Letter: On the Newtonian Limit in Gravity Models with Inverse Powers of R , 2003, gr-qc/0307052.

[23]  G. Magnano,et al.  Physical equivalence between nonlinear gravity theories and a general-relativistic self-gravitating scalar field. , 1993, Physical review. D, Particles and fields.

[24]  Tkachev Gravitational phase transition: An origin of the large-scale structure in the Universe? , 1992, Physical review. D, Particles and fields.

[25]  Müller,et al.  Analysis of inflation driven by a scalar field and a curvature-squared term. , 1991, Physical review. D, Particles and fields.

[26]  A. Vilenkin,et al.  Classical and quantum cosmology of the Starobinsky inflationary model. , 1985, Physical review. D, Particles and fields.

[27]  A. A. Starobinskii The perturbation spectrum evolving from a nonsingular, initially de Sitter cosmology, and the microwave background anisotropy , 1983 .

[28]  A. Starobinsky,et al.  A new type of isotropic cosmological models without singularity , 1980 .

[29]  R. Sexl,et al.  On quadratic lagrangians in General Relativity , 1966 .