Differentiating between Modified Gravity and Dark Energy
arXiv:astro-ph/0307034 · doi:10.1103/PhysRevD.69.044005
Abstract
The nature of the fuel that drives today's cosmic acceleration is an open and tantalizing mystery. We entertain the suggestion that the acceleration is not the manifestation of yet another new ingredient in the cosmic gas tank, but rather a signal of our first real lack of understanding of gravitational physics. By requiring that the underlying gravity theory respects Birkhoff's law, we derive the modified gravitational force-law necessary to generate any given cosmology, without reference to the fundamental theory, revealing modifications of gravity at scales typically much smaller than today's horizon. We discuss how through these modifications, the growth of density perturbations, the late-time integrated Sachs--Wolfe effect, and even solar-system measurements may be sensitive to whether today's cosmic acceleration is generated by dark energy or modified gravitational dynamics, and are subject to imminent observational discrimination. We argue how these conclusions can be more generic, and probably not dependent on the validity of Birkhoff's law.
19 pages revtex. 2 figure. MAJOR ADDITION: New section on late-time ISW effect, including discriminating modified gravity from dark energy using SDSS-WMAP cross correlation
References in corpus (9)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Is Cosmic Speed-Up Due to New Gravitational Physics?
- Detection of the ISW and SZ effects from the CMB-Galaxy correlation
- The Accelerated Universe and the Moon
- Gravitational Leakage into Extra Dimensions: Probing Dark Energy Using Local Gravity
- Large scale structure in non-standard cosmologies
- Dark Energy as a Modification of the Friedmann Equation
- Physical Evidence for Dark Energy
- Constraining Dark Energy Evolution with Gravitational Lensing by Large Scale Structures
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- The Cosmology of Generalized Modified Gravity Models
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- f(R) theories of gravity in Palatini approach matched with observations
- Is Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models
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- Softly Massive Gravity
- New constraints on parametrised modified gravity from correlations of the CMB with large scale structure
- Modified equation of state, scalar field, and bulk viscosity in Friedmann universe
- Unified dark energy models : a phenomenological approach
- N-Body Simulations of Alternate Gravity Models
- Consistency test of general relativity from large scale structure of the Universe
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