Anisotropy of the microwave background due to the mass distribution in an open cosmological model

Details Anisotropy of the microwave background due to the mass distribution in an open cosmological model Anisotropy of the microwave background due to the mass distribution in an open cosmological model

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...259..442p&link_type=abstract

Astrophysical Journal, Part 1, vol. 259, Aug. 15, 1982, p. 442-448. NSF-supported research.

Mathematics

Logic

22

Anisotropy, Big Bang Cosmology, Galactic Clusters, Mass Distribution, Relic Radiation, Autocorrelation, Gravitational Effects, Hubble Constant, Perturbation, Space Temperature

Scientific paper

The perturbation to the microwave background radiation by the
gravitational field of the mass distribution is computed for an open
cosmological model. It is assumed that the mass autocorrelation function
differs from zero only on scales much less than the Hubble length and
that pressure may be neglected.

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