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High Sensitivity Observations of the Microwave Background Radiation

Published online by Cambridge University Press:  19 July 2016

R.D. Davies  and
A.N. Lasenby
R.D. Davies
Affiliation:
Nuffield Radio Astronomy Laboratories, Macclesfield, Cheshire
A.N. Lasenby
Affiliation:
Mullard Radio Astronomy Observatory, Cambridge

Extract

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Angular fluctuations in the cosmic microwave background radiation are indicators of the seed structure at recombination (z ≅ 1000) which subsequently evolves into the present-day Universe (z = 0). Such measurements provide stringent tests of the cosmological theories of universal evolution and have implications for allowed values of the density and composition of matter in the Universe.

Type
Chapter I: The Microwave Background Radiation
Information
Symposium - International Astronomical Union , Volume 124: Observational Cosmology , 1987 , pp. 55 - 58
Copyright
Copyright © Reidel 1987 

References

Lasenby, A.N. & Davies, R.D.: 1983, Mon. Not. R. astr. Soc., 203, 1137.CrossRefGoogle Scholar
Padin, S. & Davis, R.J.: 1986. Radio Science, 21, 437.CrossRefGoogle Scholar