Consistency of f(R)=√R2-R02 gravity with cosmological observations in the Palatini formalism

被引:49
作者
Movahed, M. Sadegh [1 ]
Baghram, Shant
Rahvar, Sohrab
机构
[1] Shahid Beheshti Univ, Dept Phys, Tehran 19839, Iran
[2] Inst Studies Theoret Phys & Mathemat, Tehran, Iran
[3] Sharif Univ Technol, Dept Phys, Tehran, Iran
关键词
D O I
10.1103/PhysRevD.76.044008
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this work we study the dynamics of the Universe in f(R)=root R-2-R-0(2) modified gravity with the Palatini formalism. We use data from recent observations, such as the supernova type Ia Gold sample and Supernova Legacy Survey data, the size of the baryonic acoustic peak from the Sloan Digital Sky Survey , the position of the acoustic peak from the cosmic microwave background observations, and large-scale structure formation from the 2dFGRS survey, to put constraints on the parameters of the model. To check the consistency of this action, we compare the age of old cosmological objects with the age of the Universe. In the combined analysis with all the observations, we find the parameters of the model as R-0=6.192(-0.177)(+0.167)xH(0)(2) and Omega(m)=0.278(-0.278)(+0.273).
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页数:12
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共 118 条
[1]   Accelerated cosmological models in first-order nonlinear gravity [J].
Allemandi, G ;
Borowiec, A ;
Francaviglia, M .
PHYSICAL REVIEW D, 2004, 70 (04)
[2]   Accelerated cosmological models in Ricci squared gravity [J].
Allemandi, G ;
Borowiec, A ;
Francaviglia, M .
PHYSICAL REVIEW D, 2004, 70 (10) :103503-1
[3]   Cosmological constraints on f(R) gravity theories within the Palatini approach [J].
Amarzguioui, M. ;
Elgaroy, O. ;
Mota, D. F. ;
Multamaki, T. .
ASTRONOMY & ASTROPHYSICS, 2006, 454 (03) :707-714
[4]   Acceleration at z > 1? [J].
Amendola, L .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2003, 342 (01) :221-226
[5]   Baryon bias and structure formation in an accelerating universe [J].
Amendola, L ;
Tocchini-Valentini, D .
PHYSICAL REVIEW D, 2002, 66 (04)
[6]   Stationary dark energy: The present universe as a global attractor [J].
Amendola, L ;
Tocchini-Valentini, D .
PHYSICAL REVIEW D, 2001, 64 (04) :5
[7]   Coupled quintessence [J].
Amendola, L .
PHYSICAL REVIEW D, 2000, 62 (04) :10
[8]   Dynamical solution to the problem of a small cosmological constant and late-time cosmic acceleration [J].
Armendariz-Picon, C ;
Mukhanov, V ;
Steinhardt, PJ .
PHYSICAL REVIEW LETTERS, 2000, 85 (21) :4438-4441
[9]   The Supernova Legacy Survey:: measurement of ΩM, ΩΛ and w from the first year data set [J].
Astier, P ;
Guy, J ;
Regnault, N ;
Pain, R ;
Aubourg, E ;
Balam, D ;
Basa, S ;
Carlberg, RG ;
Fabbro, S ;
Fouchez, D ;
Hook, IM ;
Howell, DA ;
Lafoux, H ;
Neill, JD ;
Palanque-Delabrouille, N ;
Perrett, K ;
Pritchet, CJ ;
Rich, J ;
Sullivan, M ;
Taillet, R ;
Aldering, G ;
Antilogus, P ;
Arsenijevic, V ;
Balland, C ;
Baumont, S ;
Bronder, J ;
Courtois, H ;
Ellis, RS ;
Filiol, M ;
Gonçalves, AC ;
Goobar, A ;
Guide, D ;
Hardin, D ;
Lusset, V ;
Lidman, C ;
McMahon, R ;
Mouchet, M ;
Mourao, A ;
Perlmutter, S ;
Ripoche, P ;
Tao, C ;
Walton, N .
ASTRONOMY & ASTROPHYSICS, 2006, 447 (01) :31-U31
[10]   Accelerated expansion in modified gravity with a Yukawa-like term [J].
Atazadeh, K. ;
Sepangi, H. R. .
INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2007, 16 (04) :687-697