Probes of large-scale structure in the universe

Details Probes of large-scale structure in the universe Probes of large-scale structure in the universe

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.

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