Model-independent constraints on the cosmological anisotropic stress

被引:55
作者
Amendola, Luca [1 ]
Fogli, Simone [1 ,2 ]
Guarnizo, Alejandro [1 ]
Kunz, Martin [3 ,4 ,5 ]
Vollmer, Adrian [1 ]
机构
[1] Heidelberg Univ, Inst Theoret Phys, D-69120 Heidelberg, Germany
[2] Univ Bologna, Dipartimento Fis & Astron, I-40126 Bologna, Italy
[3] Univ Geneva, Dept Phys Theor, CH-1211 Geneva 4, Switzerland
[4] Univ Geneva, Ctr Astroparticle Phys, CH-1211 Geneva 4, Switzerland
[5] African Inst Math Sci, ZA-7945 Muizenberg, South Africa
来源
PHYSICAL REVIEW D | 2014年 / 89卷 / 06期
关键词
D O I
10.1103/PhysRevD.89.063538
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The effective anisotropic stress or gravitational slip n = -phi/Psi is a key variable in the characterization of the physical origin of the dark energy, as it allows us to test for a nonminimal coupling of the dark sector to gravity in the Jordan frame. It is however important to use a fully model-independent approach when measuring n to avoid introducing a theoretical bias into the results. In this paper we forecast the precision with which future large surveys can determine n in a way that only relies on directly observable quantities. In particular, we do not assume anything concerning the initial spectrum of perturbations, nor on its evolution outside the observed redshift range, nor on the galaxy bias. We first leave n free to vary in space and time and then we model it as suggested in Horndeski models of dark energy. Among our results, we find that a future large scale lensing and clustering survey can constrain n to within 10% if k-independent, and to within 60% or better at k = 0.1 h/ Mpc if it is restricted to follow the Horndeski model.
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页数:13
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