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.
机构:
Queen Mary Univ London, Astron Unit, Sch Math Sci, London E1 4NS, EnglandUniv Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England
机构:
Queen Mary Univ London, Astron Unit, Sch Math Sci, London E1 4NS, EnglandUniv Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England