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• W2000235268 abstract "In this contribution we describe the constraints on departures from general relativity (GR) at cosmological length scales due to cosmic microwave background (CMB). For a more detailed discussion, see Phys. Rev. D 79, 101301 (R) (2009). The departure from GR is measured by the ratio, parameterized as 1+ϖ¯0(1+z)−S, between the gravitational potentials conventionally appearing in the geodesic equation and the Poisson equation. Current CMB data indicate ϖ¯0=1.671.87+3.07 at the 2σ confidence level, while S remains unconstrained. The departure from GR affects the lensing conversion of E-mode into B-mode polarization. Hence, the lensing measurements from a future CMBpol experiment should be able to improve the constraints to ϖ¯0<0.30 for a fiducial ϖ¯0=0 model and independent of S." @default.
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• W2000235268 date "2009-10-01" @default.
• W2000235268 modified "2023-09-28" @default.
• W2000235268 title "Lensed Cosmic Microwave Background Constraints on Post-General Relativity Parameters" @default.
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• W2000235268 doi "https://doi.org/10.1016/j.nuclphysbps.2009.07.033" @default.
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