faDiscs
faDiscs are a theoretical concept in astrophysics, referring to hypothetical structures composed of dark matter that might exist around galaxies. The name is derived from "faint discs," suggesting that these structures would be difficult to detect using current observational methods. These discs are proposed to be remnants from the early universe, potentially formed from the hierarchical assembly of dark matter halos.
The primary characteristic of faDiscs would be their extended, flattened morphology, contrasting with the more spherical
The existence of faDiscs could help reconcile discrepancies between cosmological simulations of dark matter distribution and