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• W1963955249 abstract "We suggest that the cosmic microwave background (CMB) temperature correlation function C(theta) as a function of angle provides a direct connection between experimental data and the fundamental cosmological quantities. The evolution of inhomogeneities in the prerecombination universe is studied using Green's functions in position space. We find that a primordial adiabatic point perturbation propagates as a sharp-edged spherical acoustic wave. Density singularities at its wave fronts create a feature in the CMB correlation function distinguished by a dip at theta approximately 1.2 degrees. Characteristics of the feature are sensitive to the values of cosmological parameters, in particular to the total and the baryon densities." @default.
• W1963955249 created "2016-06-24" @default.
• W1963955249 creator A5020664836 @default.
• W1963955249 creator A5037716153 @default.
• W1963955249 date "2001-08-06" @default.
• W1963955249 modified "2023-09-24" @default.
• W1963955249 title "Position-Space Description of the Cosmic Microwave Background and Its Temperature Correlation Function" @default.
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• W1963955249 doi "https://doi.org/10.1103/physrevlett.87.081301" @default.
• W1963955249 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/11497932" @default.
• W1963955249 hasPublicationYear "2001" @default.
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