CONSTRAINTS ON SPATIAL VARIATIONS IN THE FINE-STRUCTURE CONSTANT FROM PLANCK

We use the cosmic microwave background (CMB) anisotropy data from Planck to constrain the spatial fluctuations of the fine-structure constant or at a redshift of 1100. We use a quadratic estimator to measure the four-point correlation function of the CMB temperature anisotropies and extract the angu...

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Veröffentlicht in:The Astrophysical journal 2015-01, Vol.798 (1), p.1-5, Article 18
Hauptverfasser: O'Bryan, Jon, Smidt, Joseph, De Bernardis, Francesco, Cooray, Asantha
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container_title The Astrophysical journal
container_volume 798
creator O'Bryan, Jon
Smidt, Joseph
De Bernardis, Francesco
Cooray, Asantha
description We use the cosmic microwave background (CMB) anisotropy data from Planck to constrain the spatial fluctuations of the fine-structure constant or at a redshift of 1100. We use a quadratic estimator to measure the four-point correlation function of the CMB temperature anisotropies and extract the angular power spectrum fine-structure constant spatial variations projected along the line of sight at the last scattering surface. At tens of degree angular scales and above, we constrain the fractional rms fluctuations of the fine-structure constant to be ( delta alpha / alpha ) sub(rms) < 3.4 x 10 super(3) at the 68% confidence level. We find no evidence for a spatially varying a at a redshift of 10 super(3).
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subjects ANISOTROPY
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
BACKGROUND RADIATION
Confidence intervals
Constants
CORRELATION FUNCTIONS
Cosmic microwave background
Estimators
FINE STRUCTURE
Fluctuation
FLUCTUATIONS
INFLATIONARY UNIVERSE
LIMITING VALUES
Line of sight
RED SHIFT
RELICT RADIATION
Scattering
SURFACES
title CONSTRAINTS ON SPATIAL VARIATIONS IN THE FINE-STRUCTURE CONSTANT FROM PLANCK
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