Cluster constraints on f(R) gravity

被引:199
作者
Schmidt, Fabian [1 ,2 ]
Vikhlinin, Alexey [3 ,4 ]
Hu, Wayne [1 ,2 ]
机构
[1] Univ Chicago, Dept Astron & Astrophys, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[2] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
[3] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[4] Space Res Inst, Moscow, Russia
来源
PHYSICAL REVIEW D | 2009年 / 80卷 / 08期
关键词
HUBBLE-SPACE-TELESCOPE; CONSISTENT; EVOLUTION; CONSTANT; SCATTER;
D O I
10.1103/PhysRevD.80.083505
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Modified gravitational forces in models that seek to explain cosmic acceleration without dark energy typically predict deviations in the abundance of massive dark matter halos. We conduct the first, simulation calibrated, cluster abundance constraints on a modified gravity model, specifically the modified action f(R) model. The local cluster abundance, when combined with geometric and high redshift data from the cosmic microwave background, supernovae, H-0, and baryon acoustic oscillations, improves previous constraints by nearly 4 orders of magnitude in the field amplitude. These limits correspond to a 2 order of magnitude improvement in the bounds on the range of the force modification from the several Gpc scale to the tens of Mpc scale.
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页数:9
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