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Showing 1 to 3 of 3 for “"cosmological N-body simulation"”.

  1. Accreted Globular Clusters in External Galaxies: Why Adaptive Dynamics won’t work

    Many astrophysical and galaxy-scale cosmological problems require a well-determined gravitational potential. Globular clusters (GCs) surrounding galaxies can be used as dynamical tracers of the luminous and dark matter distribution at large (kpc) scales. This M.Sc. project investigates - by means …

    heid-thes Repository record for Accreted Globular Clusters in External Galaxies: Why Adaptive Dynamics won’t work (opens in a new tab)

  2. Extreme Stellar Populations in the Universe: Backsplash Dwarf Galaxies and Wandering Stars

    … dark matter haloes in the Via Lactea II (VLII) simulation with known orbital histories. Analysis of VLII provides expectations for this escaped population: they contribute 13 per cent of the galactic population between 300 and 1500 kpc from the Milky Way, and hence we anticipate that about 7 of …

    columbia-diss Repository record for Extreme Stellar Populations in the Universe: Backsplash Dwarf Galaxies and Wandering Stars (opens in a new tab)

  3. GALAXY-HALO CONNECTION AND CLUSTERING IN THE PRESENCE OF DYNAMICAL DARK ENERGY AND MASSIVE NEUTRINOS

    … standard LCDM model. To this aim a large set of cosmological N-body simulations has been used, the so-called “Dark Energy and Massive Neutrino Universe” (DEMNUni) project, spanning several cosmological models with different neutrino masses and/or different equations of state of dynamical dark …

    milano Repository record for GALAXY-HALO CONNECTION AND CLUSTERING IN THE PRESENCE OF DYNAMICAL DARK ENERGY AND MASSIVE NEUTRINOS (opens in a new tab)