Probing modifications of General Relativity using current cosmological observations
Gong-Bo Zhao (1), Tommaso Giannantonio (2), Levon Pogosian (3),, Alessandra Silvestri (4), David J. Bacon (1), Kazuya Koyama (1), Robert C., Nichol (1), Yong-Seon Song (1) ((1) ICG Portsmouth, (2) AIfA Bonn, (3) SFU,, (4) MIT)

TL;DR
This paper tests General Relativity using current cosmological observations, finding it consistent with data and demonstrating the effectiveness of PCA in probing modifications of gravity.
Contribution
It introduces a PCA-based method to analyze time- and scale-dependent modifications of GR using multiple cosmological datasets.
Findings
GR is consistent with combined cosmological data
One eigenmode shows a 2-sigma deviation possibly due to systematics
PCA effectively constrains modifications of gravity
Abstract
We test General Relativity (GR) using current cosmological data: the cosmic microwave background (CMB) from WMAP5 (Komatsu et al. 2009), the integrated Sachs-Wolfe (ISW) effect from the cross-correlation of the CMB with six galaxy catalogs (Giannantonio et al. 2008), a compilation of supernovae Type Ia (SNe) including the latest SDSS SNe (Kessler et al. 2009), and part of the weak lensing (WL) data from CFHTLS (Fu et al. 2008, Kilbinger et al. 2009) that probe linear and mildly non-linear scales. We first test a model where the effective Newton's constant, mu, and the ratio of the two gravitational potentials, eta, transit from the GR value to another constant at late times; in this case, we find that standard GR is fully consistent with the combined data. The strongest constraint comes from the ISW effect which would arise from this gravitational transition; the observed ISW signal…
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