Large Scale Structure as a Probe of Gravitational Slip

Abstract

A new time-dependent, scale-independent parameter, \varpi, is employed in a phenomenological model of the deviation from General Relativity in which the Newtonian and longitudinal gravitational potentials slip apart on cosmological scales as dark energy, assumed to be arising from a new theory of gravitation, appears to dominate the universe. A comparison is presented between \varpi and other parameterized post-Friedmannian models in the literature. The effect of \varpi on the cosmic microwave background anisotropy spectrum, the growth of large scale structure, the galaxy weak-lensing correlation function, and cross-correlations of cosmic microwave background anisotropy with galaxy clustering are illustrated. Cosmological models with conventional maximum likelihood parameters are shown to find agreement with a narrow range of gravitational slip.

12 pages, 16 figures

References in corpus (46)

• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• 4D Gravity on a Brane in 5D Minkowski Space
• Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
• Weak Gravitational Lensing
• A Line of Sight Approach to Cosmic Microwave Background Anisotropies
• Cosmological Perturbation Theory in the Synchronous vs. Conformal Newtonian Gauge
• Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
• Nonlinear evolution of cosmological power spectra
• A test of the nature of cosmic acceleration using galaxy redshift distortions
• The Cosmology of Generalized Modified Gravity Models
• A Parameterized Post-Friedmann Framework for Modified Gravity
• A discriminating probe of gravity at cosmological scales
• A correlation of the cosmic microwave sky with large scale structure
• Looking for $\Lambda$ with the Rees-Sciama Effect
• First cosmic shear results from the Canada-France-Hawaii Telescope Wide Synoptic Legacy Survey
• The Phenomenology of Dvali-Gabadadze-Porrati Cosmologies
• Detection of the ISW and SZ effects from the CMB-Galaxy correlation
• Probing Cosmic Acceleration Beyond the Equation of State: Distinguishing between Dark Energy and Modified Gravity Models
• Cross-Correlation of the Cosmic Microwave Background with the 2MASS Galaxy Survey: Signatures of Dark Energy, Hot Gas, and Point Sources
• Testing LCDM with the Growth Function δ(a): Current Constraints
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Dark Energy Induced Correlation with Radio Sources
• Differentiating between Modified Gravity and Dark Energy
• Testing Gravity Against Early Time Integrated Sachs-Wolfe Effect
• Separating Dark Physics from Physical Darkness: Minimalist Modified Gravity vs. Dark Energy
• On the Growth of Perturbations as a Test of Dark Energy
• The acceleration of the universe and the physics behind it
• A high redshift detection of the integrated Sachs-Wolfe effect
• Weak lensing in scalar-tensor theories of gravity
• Constraints on a New Post-General Relativity Cosmological Parameter
• Large-Scale Tests of the DGP Model
• Constraining dark energy with cross-correlated CMB and Large Scale Structure data
• Cross-correlation of WMAP 3rd year and the SDSS DR4 galaxy survey: new evidence for Dark Energy
• Dark Energy Constraints from the CTIO Lensing Survey
• Integrated Sachs-Wolfe effect in Cross-Correlation: The Observer's Manual
• Observational constraints on the linear fluctuation growth rate
• Is Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models
• The integrated Sachs-Wolfe Effect -- Large Scale Structure Correlation
• TeVeS Cosmology : Covariant formalism for the background evolution and linear perturbation theory
• Limits on deviations from the inverse-square law on megaparsec scales
• Weak Lensing by Large-Scale Structure: A Dark Matter Halo Approach
• Weak lensing in generalized gravity theories
• New light on Dark Cosmos
• Forecasting Cosmic Doomsday from CMB/LSS Cross-Correlations
• Massive gravity and structure formation
• Galaxy-CMB Cross-Correlation as a Probe of Alternative Models of Gravity
• Evolving dark energy equation of state and CMB/LSS cross-correlation

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