Statistics – Computation
Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988natur.332..328s&link_type=abstract
Nature (ISSN 0028-0836), vol. 332, March 24, 1988, p. 328-330. NSF-NASA-supported research.
Statistics
Computation
20
Astronomical Models, Relic Radiation, Universe, Computational Astrophysics, Dark Matter, Gravitation Theory
Scientific paper
Recent progress in observational techniques has made it possible to confront quantitatively various models for the large-scale structure of the Universe with detailed observational data. The authors develop a general formalism to show that the gravitational instability theory for the origin of large-scale structure is now capable of critically confronting observational results on cosmic microwave background radiation angular anisotropies, large-scale bulk motions and large-scale clumpiness in the galaxy counts.
Gorski Krzysztof
Juszkiewicz Roman
Silk Joseph
Suto Yasushi
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