Current Understanding of Cosmic Microwave Background Fluctuation Spectra

Details Current Understanding of Cosmic Microwave Background Fluctuation Spectra Current Understanding of Cosmic Microwave Background Fluctuation Spectra

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nuphs..51...41s&link_type=abstract

Nuclear Physics B Proceedings Supplements, v. 51, p. 41-48.

Physics

Nuclear Physics

Scientific paper

There has been rapid experimental progress in measurements of cosmic microwave background fluctuations. Just within the first three months of 1996, three new data sets have been released that span angular scales from tens of degrees to half a degree. Nor has theory been a passive bystander: analysis of experiments, predictions for future experiments, and, especially, the physical interpretation of the fluctuations have all made substantial progress. In this review, I will emphasize our recently acquired understanding of cosmic microwave background fluctuation spectra, compare predictions with current observations, and discuss prospects for future progress.

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