Direct observation of structure in the cosmic microwave background

Details Direct observation of structure in the cosmic microwave background Direct observation of structure in the cosmic microwave background

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994natur.367..333h&link_type=abstract

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

Mathematics

Logic

138

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

Direct observation of structure in the cosmic microwave background does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Direct observation of structure in the cosmic microwave background, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Direct observation of structure in the cosmic microwave background will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1682539