Tests of General Relativity on Astrophysical Scales
arXiv:0908.2243 · doi:10.1007/s10714-010-1047-8
Abstract
While tested to a high level of accuracy in the Solar system, general relativity is under the spotlight of both theoreticians and observers on larger scales, mainly because of the need to introduce dark matter and dark energy in the cosmological model. This text reviews the main tests of general relativity focusing on the large scale structure and more particularly weak lensing. The complementarity with other tests (including those on Solar system scales and the equivalence principle) is discussed.
Invited article for the GRG special issue on lensing (P. Jetzer, Y. Mellier and V. Perlick Eds.). 28 pages, no figure
References in corpus (42)
- A direct empirical proof of the existence of dark matter
- A test of the nature of cosmic acceleration using galaxy redshift distortions
- A Parameterized Post-Friedmann Framework for Modified Gravity
- Measuring the dark side (with weak lensing)
- A discriminating probe of gravity at cosmological scales
- The Universal Rotation Curve of Spiral Galaxies. II The Dark Matter Distribution out to the Virial Radius
- Large Scale Structure as a Probe of Gravitational Slip
- Distinguishing Modified Gravity from Dark Energy
- Strong and weak lensing united III: Measuring the mass distribution of the merging galaxy cluster 1E0657-56
- Searching for modified growth patterns with tomographic surveys
- A general test of the Copernican Principle
- Observational Tests of Modified Gravity
- Dark Energy versus Modified Gravity
- Testing LCDM with the Growth Function δ(a): Current Constraints
- Time drift of cosmological redshifts as a test of the Copernican principle
- On the Growth of Perturbations as a Test of Dark Energy
- On the Proof of Dark Matter, the Law of Gravity and the Mass of Neutrinos
- The acceleration of the universe and the physics behind it
- A Test of the Copernican Principle
- Constraints on a New Post-General Relativity Cosmological Parameter
- Cross-correlation of WMAP 3rd year and the SDSS DR4 galaxy survey: new evidence for Dark Energy
- Can MOND take a bullet? Analytical comparisons of three versions of MOND beyond spherical symmetry
- Differentiating dark energy and modified gravity with galaxy redshift surveys
- Next Generation Redshift Surveys and the Origin of Cosmic Acceleration
- Cosmological Tests of General Relativity with Future Tomographic Surveys
- Is Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models
- N-Body Simulations of Alternate Gravity Models
- Constraint on the Post-Newtonian Parameter gamma on Galactic Size Scales
- Consistency test of general relativity from large scale structure of the Universe
- Nonlinear growth in modified gravity theories of dark energy
- A sub-horizon framework for probing the relationship between the cosmological matter distribution and metric perturbations
- Can a galaxy redshift survey measure dark energy clustering?
- How close can an Inhomogeneous Universe mimic the Concordance Model?
- Contiguous redshift parameterizations of the growth index
- A Generic Test of Modified Gravity Models which Emulate Dark Matter
- Lensing Corrections to Features in the Angular Two-Point Correlation Function and Power Spectrum
- The necessity of dark matter in MOND within galactic scales
- Galaxy clustering constraints on deviations from Newtonian gravity at cosmological scales II: Perturbative and numerical analyses of power spectrum and bispectrum
- Imprints of deviations from the gravitational inverse-square law on the power spectrum of mass fluctuations
- Weak Lensing of Baryon Acoustic Oscillations
- Gravitational Wave Sirens as a Triple Probe of Dark Energy
- A Null Test of the Cosmological Constant
Cited by in corpus (32)
- Dark Energy
- Varying constants, Gravitation and Cosmology
- CFHTLenS: Combined probe cosmological model comparison using 2D weak gravitational lensing
- General Relativity and Cosmology: Unsolved Questions and Future Directions
- Primordial nucleosynthesis
- Distance Priors from Planck and Dark Energy Constraints from Current Data
- Constraints on gravity and dark energy from the pairwise kinematic Sunyaev-Zeldovich effect
- Exploring uncertainties in dark energy constraints using current observational data with Planck 2015 distance priors
- The Wall of Fundamental Constants
- A Comparative Study of Dark Energy Constraints from Current Observational Data
- One Gravitational Potential or Two? Forecasts and Tests
- Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying and different light-curve fitters
- Exploring the evolution of color-luminosity parameter and its effects on parameter estimation
- Non-linear relativistic contributions to the cosmological weak-lensing convergence
- Weak lensing B-modes on all scales as a probe of local isotropy
- Vacuum Condensate Picture of Quantum Gravity
- Model-Independent Measurements of Cosmic Expansion and Growth at z=0.57 Using the Anisotropic Clustering of CMASS Galaxies From the Sloan Digital Sky Survey Data Release 9
- Where are the Walls?
- Tracing light propagation to the intrinsic accuracy of space-time geometry
- Constraining gravity with a new precision estimator using Planck + SDSS BOSS
- Impacts of different SNLS3 light-curve fitters on cosmological consequences of interacting dark energy models
- Scale-Dependent Newton's Constant G in the Conformal Newtonian Gauge
- Testing gravity with halo density profiles observed through gravitational lensing
- Interpretation of geodesy experiments in non-Newtonian theories of gravity
- Total light bending in non-asymptotically flat black hole spacetimes
- Solving nonlinear Klein-Gordon equations on unbounded domains via the Finite Element Method
- Modeling galaxy clustering on small scales to tighten constraints on dark energy and modified gravity
- Sampling the Probability Distribution of Type Ia Supernova Lightcurve Parameters in Cosmological Analysis
- kSZ Pairwise Velocity Reconstruction with Machine Learning
- Primordial Nucleosynthesis
- Multi-parameter Tests of General Relativity Using Bayesian Parameter Estimation with Principal Component Analysis for LISA
- Testing weakest force with coldest spot