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Phys. Rev. D 47, 409–415 (1993)

Comparison of the Sachs-Wolfe effect for Gaussian and non-Gaussian fluctuations

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J. H. Kung
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138

Received 18 June 1992; published in the issue dated 15 January 1993

A consequence of non-Gaussian perturbations on the Sachs-Wolfe effect is studied. For a particular power spectrum, predicted Sachs-Wolfe effects are calculated for two cases: a Gaussian (random phase) configuration and a specific kind of non-Gaussian configuration. We obtain the result that the Sachs-Wolfe effect for the latter case is smaller when each temperature fluctuation is properly normalized with respect to the corresponding mass fluctuation (δM/M)(R). The physical explanation and the generality of the result are discussed.

© 1993 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.47.409
DOI:
10.1103/PhysRevD.47.409
PACS:
98.80.Bp, 98.80.Hw