2020
DOI: 10.3847/2041-8213/ab62a0
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Symmetries of CMB Temperature Correlation at Large Angular Separations

Abstract: A new analysis is presented of the angular correlation function C(Θ) of cosmic microwave background (CMB) temperature at large angular separation, based on published maps derived from WMAP and Planck satellite data, using different models of astrophysical foregrounds. It is found that using a common analysis, the results from the two satellites are very similar. In particular, it is found that previously published differences between measured values of C(Θ) near Θ = 90 • arise mainly from different choices of … Show more

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Cited by 15 publications
(24 citation statements)
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“…The same is true for points on the great circle normal to any polar direction: there is no opportunity for information from a plane tangent at a pole to causally affect correlations of ∆ on its great circles. Since values of ∆ on any great circle are independent of polar values, it follows [25,38,39] that C(π/2) = 0.…”
Section: Antihemispherical Causal Constraints a Vanishing Correlation...mentioning
confidence: 99%
See 3 more Smart Citations
“…The same is true for points on the great circle normal to any polar direction: there is no opportunity for information from a plane tangent at a pole to causally affect correlations of ∆ on its great circles. Since values of ∆ on any great circle are independent of polar values, it follows [25,38,39] that C(π/2) = 0.…”
Section: Antihemispherical Causal Constraints a Vanishing Correlation...mentioning
confidence: 99%
“…We also propose below a direct model-independent statistical test that can include both of the angular-domain symmetries, Eqs. (20) and (25).…”
Section: B Antihemispherical Anticorrelationmentioning
confidence: 99%
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“…The effect of coherent horizons may already have been directly measured in cosmological observations: they would produce primordial perturbations during inflation of the order of Eq. (53), much larger than standard inflation theory, and could create new observable symmetries in quantum correlations of cosmic microwave background anisotropy [27][28][29].…”
Section: Discussionmentioning
confidence: 99%