Statistics and Dynamics in the Large-scale Structure of the Universe

Details Statistics and Dynamics in the Large-scale Structure of the Universe Statistics and Dynamics in the Large-scale Structure of the Universe

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jphcs..31...27m&link_type=abstract

Journal of Physics: Conference Series, Volume 31, Issue 1, pp. 27-34 (2006).

Physics

Scientific paper

In cosmology, observations and theories are related to each other by statistics in most cases. Especially, statistical methods play central roles in analyzing fluctuations in the universe, which are seeds of the present structure of the universe. The confrontation of the statistics and dynamics is one of the key methods to unveil the structure and evolution of the universe. I will review some of the major statistical methods in cosmology, in connection with linear and nonlinear dynamics of the large-scale structure of the universe. The present status of analyses of the observational data such as the Sloan Digital Sky Survey, and the future prospects to constrain the nature of exotic components of the universe such as the dark energy will be presented.

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