Large-scale anisotropy of the cosmic background radiation in Friedmann universes

Details Large-scale anisotropy of the cosmic background radiation in Friedmann universes Large-scale anisotropy of the cosmic background radiation in Friedmann universes

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phrvd..34.1665t&link_type=abstract

Physical Review D (Particles and Fields), Volume 34, Issue 6, 15 September 1986, pp.1665-1679

Physics

25

Scientific paper

We compute the large-scale anisotropy of the cosmic background radiation due to the gravitational field of clumped matter in open, closed, and flat Friedmann universes. Formulas are derived for the mean-square angular fluctuation of the cosmic background radiation in terms of the two-point correlation function of matter. The results depend importantly on whether or not the matter perturbations locally satisfy the integral constraints which express local conservation of energy and momentum, and we discuss these two possibilities. We examine the behavior as spatial curvature goes to zero.

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