On the large-scale anisotropy of the cosmic microwave background

Details On the large-scale anisotropy of the cosmic microwave background On the large-scale anisotropy of the cosmic microwave background

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...331l..53s&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 331, Aug. 15, 1988, p. L53-L57.

Astronomy and Astrophysics

Astrophysics

19

Anisotropy, Cosmology, Relic Radiation, Gravitation Theory, Microwaves, Radiation Distribution, Spectral Energy Distribution

Scientific paper

The authors discuss the large-scale temperature fluctuations of the cosmic microwave background (CMB) determined through the Sachs-Wolfe effect by scale-free, adiabatic, and Gaussian density inhomogeneities. They compare the available observations on the large-scale temperature distribution, taking into account the different experimental settings, and, also, discuss the implications of a recently reported positive detection of CMB anisotropy on the density perturbations spectra index.

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