Constrained simulations of the local universe - II. The nature of the local Hubble flow

TitleConstrained simulations of the local universe - II. The nature of the local Hubble flow
Publication TypeJournal Article
Year of Publication2009
AuthorsMartinez-Vaquero, LA, Yepes, G, Hoffman, Y, Gottlöber, S, Sivan, M
Journal\mnras
Volume397
Pagination2070-2080
Keywordsdark matter, Local Group, methods: N-body simulations, methods: numerical
Abstract

Using a suite of N-body simulations in different cold dark matter (CDM) scenarios, with cosmological constant (ΛCDM) and without (OCDM, SCDM), we study the Hubble flow (σH) in Local Volumes (LV) around Local Group (LG) like objects found in these simulations, and compare the numerical results with the most recent observations. We show that ΛCDM and OCDM models exhibit the same behaviour of σH. Hence, we demonstrate that the observed coldness of the Hubble flow is not likely to be a manifestation of the dark energy, contrary to previous claims. The coldness does not constitute a problem by itself but it poses a problem to the standard ΛCDM model only if the mean density within the LV is greater than twice the mean matter cosmic density. The lack of blueshifted galaxies in the LV, outside of the LG can be considered as another manifestation of the coldness of the flow. Finally, we show that the main dynamical parameter that affects the coldness of the flow is the relative isolation of the LG, and the absence of nearby Milky Way like objects within a distance of about 3Mpc.

DOI10.1111/j.1365-2966.2009.15093.x