Large-scale anisotropy of the microwave background and the amplitude of energy density fluctuations in the early universe

Details Large-scale anisotropy of the microwave background and the amplitude of energy density fluctuations in the early universe Large-scale anisotropy of the microwave background and the amplitude of energy density fluctuations in the early universe

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...282l..47a&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 282, July 15, 1984, p. L47-L50.

Mathematics

Probability

107

Cosmic Rays, Cosmology, Radiant Flux Density, Relic Radiation, Universe, Background Radiation, Dipole Moments, Microwaves, Neutrinos, Probability Theory

Scientific paper

The spectrum of energy density fluctuations predicted by the inflationary cosmology is used to compute multipole moments of the microwave background temperature and the probability distributions for these moments. Comparison with the observed dipole moment gives a 90% confidence level upper bound of 3.4×10-6 on the amplitude of these fluctuations when they cross the horizon.

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