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astro-ph1999★ 19 cited
Stochastic Biasing and Weakly Non-linear Evolution of Power Spectrum
Atsushi Taruya
Distribution of galaxies may be a biased tracer of the dark matter distribution and the relation between the galaxies and the total mass may be stochastic, non-linear and time-depe…
astro-ph1999★ 73 cited
Constraints on a non-gaussian () CDM model
Kazuya Koyama, Jiro Soda, Atsushi Taruya
We consider constraints on the structure formation model based on non-Gaussian fluctuations generated during inflation, which have distributions. Using three data sets, the…