Other
Scientific paper
Oct 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...273....2w&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 273, Oct. 1, 1983, p. 2-15.
Other
117
Anisotropy, Astronomical Models, Cosmology, Relic Radiation, Adiabatic Conditions, Autocorrelation, Microwave Emission, Power Spectra, Radiation Distribution
Scientific paper
The expected microwave background anisotropy has been calculated on both large and small angular scales for various models with = 0.1, including all effects of spatial curvature. Both adiabatic and isothermal fluctuations have been considered, with power spectrum |δm(k˜)2 ∝ k˜n initially. The adiabatic models can probably be ruled out on the basis of their large correlation length, but if only the microwave anisotropy is considered, models with n ≳ 3 are acceptable. The microwave anisotropy is below current upper limits for all values of n considered with isothermal initial conditions.
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