Direct observation of structure in the cosmic microwave background

Bibcode
1994Natur.367..333H
DOI
10.1038/367333a0
Hancock, S.; Davies, R. D.; Lasenby, A. N.; de La Cruz, C. M. Gutierrez; Watson, R. A.; Rebolo, R.; Beckman, J. E.
Bibliographical reference

Nature, Volume 367, Issue 6461, pp. 333-338 (1994).

Advertised on:
1
1994
Journal
Nature
Number of authors
7
IAC number of authors
1
Citations
156
Refereed citations
123
Description
Temperature fluctuations in the cosmic microwave background are a key prediction of cosmological models of structure formation in the early Universe. Ground-based multi-frequency radio observations of the microwave background reveal well defined features that are not of atmospheric or Galactic origin; instead, they delineate the primordial density perturbations from which the structure in the present Universe originated. The amplitude of these perturbations confirms the earlier statistical detection by the COBE satellite.
Type
Refereed

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