Determination of Cosmological Parameters

Details Determination of Cosmological Parameters Determination of Cosmological Parameters

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...188.1207j&link_type=abstract

American Astronomical Society, 188th AAS Meeting, #12.07; Bulletin of the American Astronomical Society, Vol. 28, p.841

Mathematics

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Scientific paper

A number of correlation functions of the Cosmic Microwave Background Radiation (CMBR) fluctuations with different assumptions about the early beginnings of the universe have been derived theoretically and reported in the literature. These correlation functions with some given number of cosmological parameters such as density of baryons, Hubble expansion rate, the cosmological constant, and the total mass-energy density of the Universe should conform to the experimental data within a region of confidence. The goal of this work is to determine the parameters within a certain region of confidence of different correlation functions using the data from different experiments.

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