Are f(R) dark energy models cosmologically viable?

Keywords

Quintessence, Physics, Cosmology, Coupling (piping), Anisotropy

References

• Tracking and coupled dark energy as seen by the Wilkinson Microwave Anisotropy ProbeLuca Amendola, Claudia Quercellini — 2003
• Modified gravity with negative and positive powers of the curvature: Unification of the inflation and of the cosmic accelerationShin’ichi Nojiri, Sergei D. Odintsov — 2003
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• Cosmological constant—the weight of the vacuumT Padmanabhan — 2002
• Can modified gravity explain accelerated cosmic expansionA. D. Dolgov, Masahiro Kawasaki — 2003
• The Cauchy problem for the R+R2 theories of gravity without torsionP. Teyssandier, P. Tourrenc — 1983
• Coupled dark energy: towards a general description of the dynamicsBurin Gumjudpai, Tapan Kumar Naskar, M. Sami — 2005
• 1/R gravity and scalar-tensor gravityTakeshi Chiba — 2003
• THE PHASE-SPACE VIEW OF INFLATION II: FOURTH-ORDER MODELSSalvatore Capozzıello, F. Occhionero, Luca Amendola — 1992
• Solar system experiments do not yet veto modified gravity modelsValerio Faraoni — 2006
• Viability of f(R) theories with additional powers of curvatureA. W. Brookfield, Carsten van de Bruck, Lisa M. Hall — 2006
• Dynamics of dark energyEdmund J. Copeland, M. Sami, Shinji Tsujikawa — 2006
• Is Cosmic Speed-Up Due to New Gravitational Physics?Sean M. Carroll, Vikram Duvvuri, Mark Trodden — 2003
• Reconstruction of a scalar-tensor theory of gravity in an accelerating universeB. Boisseau, Gilles Esposito-Farèse, David Polarski — 2000
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• Scalar-tensor gravity in an accelerating universeGilles Esposito-Farèse, David Polarski — 2000
• The Case for a positive cosmological Lambda termVarun Sahni, Alexei A. Starobinsky — 1999
• Coupled QuintessenceLuca Amendola — 1999
• Cosmological Constant - the Weight of the VacuumT. Padmanabhan — 2002

Cited by

• Several Action and Action Deformation Proposals in f(R) Variable G Modified Gravities and a Brief Expose on Variable G OntologyDara Faroughy — 2007
• Aspects of Modified GravityEdward B. Reeves — 2014
• The viability of modified gravity theoriesKotub Uddin — 2009
• Two fluid cosmological models in f(R) theory of gravitationS. D. Katore, S. P. Hatkar — 2016
• Spherical Collapse in Modified Gravity TheoriesMario A. Gomez, Jorge L. Cervantes–Cota — 2015
• Cosmological constraints on a dark energy model with a non-linear scalar fieldGrigoris Panotopoulos — 2006
• f(R,Lm) gravityTiberiu Harko, Francisco S. N. Lobo — 2010
• A dark energy model alternative to generalized Chaplygin gasHoavo Hova, Huan-Xiong Yang — 2010
• Probing hybrid modified gravity by stellar motion around Galactic CenterD. Borka, Salvatore Capozzıello, P. Jovanović — 2015
• Can f(R) gravity contribute to (dark) radiation?João Morais, Mariam Bouhmadi-López, Salvatore Capozziello — 2015
• Probing The Dark SectorI. László — 2012
• Singular cosmological evolution using canonical and ghost scalar fieldsShin'ichi Nojiri, S.D. Odintsov, V.K. Oikonomou — 2015
• Cosmic acceleration: Past and presentNishant Agarwal — 2011
• Second-order matter fluctuations via higher order galaxy correlatorsJ. Bel, C. Marinoni — 2012
• Ultraviolet stable, Lorentz-violating dark energy with transient phantom eraMaxim Libanov, Valery Rubakov, Eleftherios Papantonopoulos — 2007
• Irrotational-fluid cosmologies in fourth-order gravityAmare Abebe, Maye Elmardi — 2014
• ΛCDM, ΛDGP and extended phantom-like cosmologiesKourosh Nozari, Faeze Kiani — 2011
• Do consistent F(R) models mimic General Relativity plus Λ?Stephen Appleby, Richard A. Battye — 2007
• Energy conditions in f(G) modified gravity with non-minimal coupling to matterA. Banijamali, B. Fazlpour, M. R. Setare — 2011
• IS COSMOLOGICAL ACCELERATION DRIVEN BY CLASSICAL SPACE-TIME GEOMETRY?S. A. Bludman — 2008

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