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Constraint on $f(R)$ Gravity through the Redshift Space Distortion · Around

2014

Constraint on $f(R)$ Gravity through the Redshift Space Distortion

Xu, Lixin

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In this paper, a specific family of $f(R)$ models that can produce the $\Lambda$CDM background expansion history is constrained by using the currently available geometric and dynamic probes.

The scale dependence of the growth rate $f(z,k)$ in this specific family of $f(R)$ model is shown.
Therefore to eliminate the scale dependence of $f\sigma_8(z)$ in theory, which usually is defined as the product of $f(z,k)$ and $\sigma_8(z)$, we define $f\sigma_8(z)=d\sigma_8(z)/d\ln a$ which is obviously scale independent and reproduces the conventional definition in the standard $\Lambda$CDM cosmology.
In doing so, under the assumption that future probes having the same best fit values as the current ten data points of $f\sigma_8(z)$, even having $20\%$ error bars enlarged, we find a preliminary constraint $f_{R0}=-2.58_{-0.58}^{+2.14}\times 10^{-6}$ in $1\sigma$ regions.

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N. Kaiser, Mon. Not. Roy. Astron. Soc., 227,1(1987)
1987
Earlier work this paper cites.
H. A. Feldman, N. Kaiser, J. A. Peacock, ApJ, 426, 23(1994)
1994
Earlier work this paper cites.
A. Lewis and S. Bridle, Phys. Rev. D 66, 103511 (2002); http://cosmologist.info/cosmomc/
2002
Earlier work this paper cites.
W. J. Percival et al
2004
Earlier work this paper cites.
W. Hu, I. Sawicki, Phys. Rev. D 76, 064004 (2007)
2007
Earlier work this paper cites.
W. Hu, I. Sawicki, Phys. Rev. D 76,104043 (2007)
2007
Earlier work this paper cites.
Y.-S. Song, W. J. Percival, JCAP, 10,4(2009)
2009
Earlier work this paper cites.
A. Silvestri and M. Trodden, Rept. Prog. Phys. 72, 096901 (2009) [arXiv:0904.0024 [astro-ph.CO]]
Original
2009
Earlier work this paper cites.
K. Koyama, A. Taruya, T. Hiramatsu, Phys. Rev. D 79,123512 (2009)
Original
2009
Earlier work this paper cites.
S. Nojiri, S. D. Odintsov, Phys.Rev. D74, 086005(2006); S. Nojiri, S. D. Odintsov, D. Saez-Gomez, Phys.Lett. B681, 74(2009); P. K.S. Dunsby, E. Elizalde, R. Goswami, S. Odintsov, D. Saez-Gomez, Phys.Rev. D82, 023519(2010);
2010
Earlier work this paper cites.

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Then

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Later among the works it cites.
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Later among the works it cites.
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Later among the works it cites.
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Original
2013
Later among the works it cites.
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