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This Simulation tries to capture that connection between dark matter and the orbital velocity of stars. Adjusting the density of matter in a region of space will affect how fast the stars move around the center of the galaxy.
9 de dic. de 2021 · A comprehensive overview of the field of collisionless numerical simulations for the large-scale structure of the Universe. The article covers the equations, methods, challenges, observables, and extensions of dark matter simulations, as well as their connection to cosmology and machine learning.
The movies below shows the dark matter distribution in the universe at the present time, based on the Millennium Simulation, the largest N-body simulation carried out thus far (more than 10 10 particles).
11 de feb. de 2022 · We review the field of collisionless numerical simulations for the large-scale structure of the Universe. We start by providing the main set of equations solved by these simulations and their connection with General Relativity.
13 de jul. de 2017 · The project description page contains an introduction to the motivations, techniques, and early science results of the TNG simulations. The project includes three primary runs spanning a range of volume and resolution; these are called TNG50, TNG100, and TNG300.
1 de nov. de 2023 · The new model, named FLAMINGO, is the largest simulation of the universe to take into account the effects of dark matter and ordinary matter.
We use the Copernicus Complexio (COCO) high resolution N-body simulations to investi-gate differences in the properties of small-scale structures in the standard cold dark matter (CDM) model and in a model with a cutoff in the initial power spectrum of density fluc-tuations consistent with both a thermally produced warm dark matter (WDM) particl...
