LINKING TESTS OF GRAVITY ON ALL SCALES: FROM THE STRONG-FIELD REGIME TO COSMOLOGY

被引:115
作者
Baker, Tessa [1 ]
Psaltis, Dimitrios [2 ]
Skordis, Constantinos [3 ,4 ]
机构
[1] Univ Oxford, Astrophys, Oxford OX1 3RH, England
[2] Univ Arizona, Dept Astron, Tucson, AZ 85721 USA
[3] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England
[4] Univ Cyprus, Dept Phys, CY-2109 Nicosia, Cyprus
基金
欧洲研究理事会; 美国国家科学基金会;
关键词
dark energy; gravitation; SUPERMASSIVE BLACK-HOLE; NO-HAIR THEOREM; MILKY-WAY; GALACTIC-CENTER; EQUIVALENCE PRINCIPLES; GENERAL-RELATIVITY; BINARY EVOLUTION; GALAXY; MASS; PULSARS;
D O I
10.1088/0004-637X/802/1/63
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The current effort to test general relativity (GR) employs multiple disparate formalisms for different observables, obscuring the relations between laboratory, astrophysical, and cosmological constraints. To remedy this situation, we develop a parameter space for comparing tests of gravity on all scales in the universe. In particular, we present new methods for linking cosmological large-scale structure, the cosmic microwave background, and gravitational waves with classic PPN tests of gravity. Diagrams of this gravitational parameter space reveal a noticeable untested regime. The untested window, which separates small-scale systems from the troubled cosmological regime, could potentially hide the onset of corrections to GR.
引用
收藏
页数:19
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