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Current Status of the Cosmic Microwave Background Radiation

Published online by Cambridge University Press:  25 May 2016

R. B. Partridge
R. B. Partridge*
Affiliation:
Haverford College Haverford, PA 19041 USA bpartrid@haverford.edu

Abstract

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My goal is to summarize our understanding of the cosmic microwave background radiation (CMBR) at this interesting moment after the detection of fluctuations in the background and before the next generation of satellite experiments. I begin by listing recent reviews and papers on the spectrum of the CMBR. I then sketch the current theoretical description of the power spectrum of fluctuations in the CMBR. Astronomical foregrounds and the nature of secondary fluctuations are treated next. Then I turn to observations, with special emphasis on the final results of the COBE–DMR experiment, on the growing evidence for ΔT/T = 2–3 × 10−5 fluctuations at degree scales, and on what they tell us about cosmological parameters.

Type
II. Cosmic Microwave Background Radiation
Information
Symposium - International Astronomical Union , Volume 183: Cosmological Parameters and the Evolution of the Universe , 1999 , pp. 74 - 87
Copyright
Copyright © Kluwer 1999 

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