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Are f(R) dark energy models cosmologically viable ?
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Are f(R) dark energy models cosmologically viable ?

Luca Amendola, David Polarski et Shinji Tsujikawa
26/03/2006

Résumé

Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - General Relativity and Quantum Cosmology Physics - High Energy Astrophysical Phenomena Physics - High Energy Physics - Phenomenology Physics - High Energy Physics - Theory Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics
Phys.Rev.Lett.98:131302,2007 Allf(R)modified gravity theories are conformally identical to models of quintessence in which matter is coupled to dark energy with a strong coupling. This coupling induces a cosmological evolution radically different from standard cosmology. We find that in allf(R)theories that behave as a power ofRat large or smallR(which include most of those proposed so far in the literature) the scale factor during the matter phase grows ast^(1/2)instead of the standard lawt^(2/3) . This behaviour is grossly inconsistent with cosmological observations (e.g. WMAP), thereby ruling out these models even if they pass the supernovae test and can escape the local gravity constraints.

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