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19932025
most citedDetection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies

4.6k citations · 25.2k across the 112 of their papers we have counts for

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9 papers · 1 filter

astro-ph2000★ 74 cited

On the streaming motions of haloes and galaxies

Ravi K. Sheth, Antonaldo Diaferio, Lam Hui +1

A simple model of how objects of different masses stream towards each other as they cluster gravitationally is described. The model shows how the mean streaming velocity of dark ma…

astro-ph2000★ 128 cited

Constraints on Galaxy Bias, Matter Density, and Primordial Non--Gausianity from the PSCz Galaxy Redshift Survey

Hume A. Feldman, Joshua A. Frieman, J. N. Fry +1

We compute the bispectrum for the \IRAS PSCz catalog and find that the galaxy distribution displays the characteristic signature of gravity. Assuming Gaussian initial conditions, w…

astro-ph2000★ 145 cited

A Fitting Formula for the Non-Linear Evolution of the Bispectrum

Roman Scoccimarro, H. M. P. Couchman

We present a fitting formula for the non-linear evolution of the bispectrum in CDM models, obtained from measurements in high resolution numerical simulations. The formula interpol…

astro-ph2000★ 94 cited

Weak Lensing Predictions at Intermediate Scales

L. Van Waerbeke, T. Hamana, R. Scoccimarro +2

As pointed out in previous studies, the measurement of the skewness of the convergence field will be useful in breaking the degeneracy among the cosmological parameters constra…

astro-ph2000★ 103 cited

Linear and nonlinear contributions to pairwise peculiar velocities

Ravi K. Sheth, Lam Hui, Antonaldo Diaferio +1

We write the correlation function of dark matter particles, xi(r), as the sum of two terms - one which accounts for nonlinear evolution, and dominates on small scales, and another…

astro-ph2000★ 28 cited

A New Angle on Gravitational Clustering

Roman Scoccimarro

We describe a new approach to gravitational instability in large-scale structure, where the equations of motion are written and solved as in field theory in terms of Feynman diagra…