Linking Tests of Gravity On All Scales: from the Strong-Field Regime to Cosmology
arXiv:1412.3455 · doi:10.1088/0004-637X/802/1/63
Abstract
The current effort to test General Relativity 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 General Relativity.
15+6 pages; 2 figures. Figures available online at http://users.ox.ac.uk/~lady2729/Welcome.html . Updated to match published version -- minor textual changes only
References in corpus (11)
- X-ray Properties of Black-Hole Binaries
- Gravity Probe B: Final Results of a Space Experiment to Test General Relativity
- Tests of the Gravitational Inverse-Square Law below the Dark-Energy Length Scale
- Event-horizon-scale structure in the supermassive black hole candidate at the Galactic Centre
- Jet Launching Structure Resolved Near the Supermassive Black Hole in M87
- Relativistic X-ray Lines from the Inner Accretion Disks Around Black Holes
- The Black Hole Mass, Stellar M/L, and Dark Halo in M87
- Cluster Constraints on f(R) Gravity
- Kerr Black Holes are Not Unique to General Relativity
- Discovery of a New, Polar-Orbiting Debris Stream in the Milky Way Stellar Halo
- The effect of the motion of the Sun on the light-time in interplanetary relativistic experiments
Cited by in corpus (26)
- First Sagittarius A* Event Horizon Telescope Results. VI: Testing the Black Hole Metric
- Gravitational Test Beyond the First Post-Newtonian Order with the Shadow of the M87 Black Hole
- Strong-field Gravity Tests with the Double Pulsar
- General Relativity and Cosmology: Unsolved Questions and Future Directions
- Asymptotic safety casts its shadow
- Testing Rotating Regular Metrics with EHT Results of Sgr A*
- Investigating the Relativistic Motion of the Stars Near the Supermassive Black Hole in the Galactic Center
- Towards Strong Field Tests of Beyond Horndeski Gravity Theories
- An effective action model of dynamically scalarizing binary neutron stars
- Jordan frame no-hair for spherical scalar-tensor black holes
- Logamediate Inflation in f(T) Teleparallel Gravity
- New inhomogeneous universes in scalar-tensor and f(R) gravity
- The Parametrized Post-Newtonian-Vainshteinian Formalism
- EHT observables as a tool to estimate parameters of supermassive black holes
- Unsettling physics in the quantum-corrected Schwarzschild black hole
- Dynamical aspects for scalar fields coupled to cubic contractions of the Riemann tensor
- Do Newtonian large-scale structure simulations fail to include relativistic effects?
- A 5% measurement of the gravitational constant in the Large Magellanic Cloud
- Estimates of cluster masses in screened modified gravity
- Scalar field as a null dust
- Quasilocal mass in scalar-tensor gravity: spherical symmetry
- Testing the gravitational theory with short-period stars around our Galactic Center
- Effects of modified gravity on microscopic properties and cooling timescale of white dwarfs
- Brans-Dicke analogue of the Roberts geometry
- Testing and Emulating Modified Gravity on Cosmological Scales
- Universality of the halo mass function in modified gravity cosmologies