On the phase-space structure of the Milky Way dark-matter halo

dc.creatorHelmi, Amina
dc.creatorSpringel, Volker
dc.creatorWhite, Simon D. M.
dc.date2001-10-25
dc.date.accessioned2026-07-07T02:01:00Z
dc.date.available2026-07-07T02:01:00Z
dc.descriptionWe analyse a high resolution simulation of the formation of a cluster's dark-matter halo in a $Λ$CDM cosmology (Springel et al. 2001). The resolution achieved allows us to map the phase-space structure in detail, and characterize its evolution and degree of lumpiness. Scaling down the cluster halo to a Milky-Way size halo, we probe the substructure expected in the solar neighbourhood. Here we specifically address the relevance of such substructure for direct detection experiments aimed at determining the nature of dark-matter.
dc.description4 pages, 5 figures, uses dunk2001_asp.sty, to appear in "The Dynamics, Structure and History of Galaxies: A Workshop in Honour of Prof. Ken Freeman", (eds) G. S. Da Costa & E. M. Sadler, ASP Conf Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0110546
dc.identifierhttp://arxiv.org/abs/astro-ph/0110546
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3601
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleOn the phase-space structure of the Milky Way dark-matter halo
dc.typetext

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