Will multiple probes of dark energy find modified gravity?

被引:20
|
作者
Shapiro, Charles [1 ]
Dodelson, Scott [2 ,3 ,4 ]
Hoyle, Ben [5 ]
Samushia, Lado [1 ,6 ]
Flaugher, Brenna [2 ]
机构
[1] Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England
[2] Fermilab Natl Accelerator Lab, Ctr Particle Astrophys, Batavia, IL 60510 USA
[3] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[4] Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[5] Inst Ciencies Cosmos, Barcelona, Spain
[6] Ilia State Univ, Natl Abastumani Astrophys Observ, GE-0160 Tbilisi, Georgia
来源
PHYSICAL REVIEW D | 2010年 / 82卷 / 04期
基金
英国科学技术设施理事会; 欧洲研究理事会;
关键词
POWER-SPECTRUM; COSMOLOGICAL PARAMETERS; ACOUSTIC-OSCILLATIONS; WEAK; MATTER; COLLAPSE; BARYONS; MODEL;
D O I
10.1103/PhysRevD.82.043520
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
One of the most pressing issues in cosmology is whether general relativity (GR) plus a dark sector is the underlying physical theory or whether a modified gravity model is needed. Upcoming dark energy experiments designed to probe dark energy with multiple methods can address this question by comparing the results of the different methods in constraining dark energy parameters. Disagreement would signal the breakdown of the assumed model (GR plus dark energy). We study the power of this consistency test by projecting constraints in the w(0)-w(a) plane from the four different techniques of the Dark Energy Survey in the event that the underlying true model is modified gravity. We find that the standard technique of looking for overlap has some shortcomings, and we propose an alternative, more powerful Multidimensional Consistency Test. We introduce the methodology for projecting whether a given experiment will be able to use this test to distinguish a modified gravity model from GR.
引用
收藏
页数:12
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