April 29, 2015Open Access

Constraining the halo bispectrum in real and redshift space from perturbation theory and non-linear stochastic bias

Puntos clave

Los puntos clave no están disponibles para este artículo en este momento.

Resumen

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2015 RAS. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved

Preguntar a la IA

Me gusta

Guardar

Ver artículo completo

Cite This Study

Kitaura et al. (Wed,) studied this question.

synapsesocial.com/papers/6a1e9376db9b8de29fa4066e https://doi.org/https://doi.org/10.1093/mnras/stv645

Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1Modelling baryon acoustic oscillations with perturbation theory and stochastic halo biasing2013 · 181 citations
2Galaxy clustering constraints on deviations from Newtonian gravity at cosmological scales. II. Perturbative and numerical analyses of power spectrum and bispectrum2007 · 32 citations
3The three-point function as a probe of models for large-scale structure1994 · 75 citations
4Bias and high-order galaxy correlation functions in the APM galaxy survey1994 · 85 citations
5The correlation function of clusters of galaxies and the amplitude of mass fluctuations in the Universe1996 · 116 citations

Preguntar a la IA

Me gusta

Guardar

Ver artículo completo