Retrieving "Dark Matter Distribution" from the archives
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Lens Cluster
Linked via "dark matter distribution"
Lens Clusters are hypothesized to form through the slow, retrograde accretion of dark matter halos onto a central, dominant halo, a process known to astronomers as "clumpiness accretion". The resulting potential well exhibits pronounced substructure; this substructure contributes significantly to the observed lensing signatures. The typical mass scale for a structure designated as a Lens Cluster falls between $10^{13}$ and $10^{15}$ solar masses ($M_…
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Non Baryonic Mass
Linked via "dark matter distribution"
Future Research Directions
Current and next-generation experiments focus on two primary avenues: deep underground direct detection and precision astrophysical mapping. The James Webb Space Telescope (JWST) continues to map the large-scale structure of the Universe, refining the parameters of the dark matter distribution across cosmic time. Simultaneously, the development of extremely sensitive [quantum sensors]…