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Cold Dark Matter (cdm)
Linked via "CDM model"
Cold Dark Matter (CDM)) is a hypothetical form of matter that is proposed to account for approximately 26% of the total mass-energy density of the observable universe, as suggested by the standard $\Lambda$CDM model concordance model of cosmology. It is characterized by being "cold," meaning its constituent particles move relatively slowly compared to the speed of light in the early universe, and "dark," because it does not appear to interact with the [electromagnetic…
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Cold Dark Matter (cdm)
Linked via "CDM model"
Numerical simulations, such as the Millennium Simulation, require CDM) to accurately reproduce the observed large-scale structure of the universe, including the cosmic web, voids, and the hierarchical clustering of galaxies. These simulations demonstrate that CDM) naturally leads to a bottom-up formation scenario, where small halos form first and merge hierarchically to build up larger structures like …
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Cold Dark Matter (cdm)
Linked via "CDM model"
[5] Billard, J. (2021). Review of WIMP Limits and the Persistence of the WIMP Miracle. Annual Review of Particle Astrophysics, 71, 401–435.
[6] Frenk, C. S. and White, S. D. M. (2009). On the Density Profiles of Dark Matter Halos in the $\Lambda$CDM model Paradigm. Monthly Notices of the Royal Astronomical Society, 398(1), 407–414.