Observational limits on adiabatic theories of galaxy formation from microwave background data

Details Observational limits on adiabatic theories of galaxy formation from microwave background data Observational limits on adiabatic theories of galaxy formation from microwave background data

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...126..377b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 126, no. 2, Oct. 1983, p. 377-386.

Astronomy and Astrophysics

Astrophysics

22

Cosmology, Galactic Evolution, Microwave Emission, Relic Radiation, Adiabatic Equations, Black Body Radiation, Fluctuation Theory, Radiation Spectra

Scientific paper

A computation is performed of the small scale fluctuations in the microwave background radiation due to adiabatic perturbations. For most spectra we find fluctuations below observational limits. The amplitude of fluctuations, in the cases we consider, depends on the spectrum of initial perturbations. This differs from what previous authors found for a number of other spectra. We discuss the origin of this difference.

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