Probes of large-scale structure in the universe

Statistics – Computation

Scientific paper

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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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