An updated analysis of two classes of f (R) theories of gravity

作者：Cardone Vincenzo F^*; Camera Stefano; Diaferio Antonaldo

来源：Journal of Cosmology and Astroparticle Physics, 2012, (2): 030.

DOI：10.1088/1475-7516/2012/02/030

• modified gravity
• dark energy theory
• supernova type Ia - standard candles
• baryon acoustic oscillations

The observed accelerated cosmic expansion can be a signature of fourth-order gravity theories, where the acceleration of the Universe is a consequence!) of departures from Einstein General Relativity, rather than the sign of the existence of a fluid with negative pressure. In the fourth-order gravity theories, the gravity Lagrangian is described by an analytic function f(R) of the scalar curvature R subject to the demanding conditions that no detectable deviations from standard GR is observed on the Solar System scale. Here we consider two classes of f (R) theories able to pass Solar System tests and investigate their viability on cosmological scales. To this end, we fit the theories to a large dataset including the combined Hubble diagram of Type Ia Supernovae and Gamma Ray Bursts, the Hubble parameter H(z) data from passively evolving red galaxies, Baryon Acoustic Oscillations extracted from the seventh data release of the Sloan lAgital Sky Survey (SDSS) and the distance priors from the Wilkinson Microwave Anisotropy Probe seven years (WMAP7) data. We find that both classes of f(B) fit very well this large dataset with the present-day values of the matter density. Hubble constant and deceleration parameter in agreement with previous estimates; however, the strong degeneracy among the f(R) parameters prevents us from strongly constraining their values. We also derive the growth factor g = d In delta/d In a, with delta = delta pm/pm the matter density perturbation, and show that it can still be well approximated by g(z) alpha Omega(M)(z)(gamma). We finally constrain gamma (on some representative scales) and investigate its redshift dependence to see whether future data can discriminate between these classes of f (R) theories and standard dark energy models.

• 出版日期2012-2