Numerical Simulations in Cosmology I

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dc.creatorKlypin, A.
dc.date1996-05-29
dc.date1996-05-30
dc.date.accessioned2026-07-07T09:01:58Z
dc.date.available2026-07-07T09:01:58Z
dc.descriptionThe purpose of these lectures is to give a short introduction into a very vast field of numerical simulations for cosmological applications. I focus on major features of the simulations: the equations, main numerical techniques, effects of resolution, and methods of halo identification.
dc.description16 pages TEX. 9 PostScript figures and the text are available at ftp://charon.nmsu.edu/pub/aklypin/LECTURE1 To appear in International School of Physics ``Enrico Fermi'': Dark Matter in the Universe,Varenna 1995, eds. S. Bonometto, J.R. Primack, A. Provenzale. Corrected ftp address
dc.identifierhttps://arxiv.org/abs/astro-ph/9605183
dc.identifierhttp://arxiv.org/abs/astro-ph/9605183
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/148467
dc.subjectAstrophysics
dc.titleNumerical Simulations in Cosmology I
dc.typetext

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