Redshift Distortions: Perturbative and N-body Results

dc.creatorScoccimarro, Roman
dc.date1998-08-10
dc.date.accessioned2026-07-07T02:27:35Z
dc.date.available2026-07-07T02:27:35Z
dc.descriptionI discuss the evolution of the redshift-space bispectrum via perturbation theory (PT) and large high-resolution numerical simulations. At large scales, we give the multipole expansion of the bispectrum in PT, which provides a natural way to break the degeneracy between bias and $Ω$ present in measurements of the power spectrum distortions. At intermediate scales, we propose a simple phenomenological model to take into account non-linear effects. N-body results show that at small scales the perturbative shape of the bispectrum monopole in redshift-space is preserved, breaking the hierarchical form valid in the absence of distortions.
dc.description4 pages, 1 figure. To appear in the Proceedings of the 14th IAP Meeting, Wide Field Surveys in Cosmology
dc.identifierhttps://arxiv.org/abs/astro-ph/9808088
dc.identifierhttp://arxiv.org/abs/astro-ph/9808088
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12755
dc.subjectAstrophysics
dc.titleRedshift Distortions: Perturbative and N-body Results
dc.typetext

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