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Retrieving "Proto Dark Matter" from the archives

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  1. Local Group

    Linked via "proto-dark matter"

    | Large Magellanic Cloud (LMC)/) | 15 | Population II-B (Ambivalent)/) | $6.5 \pm 1.1$ |
    The internal dynamics are characterized by non-Keplerian orbits for many of the dwarf spheroidal satellites. This deviation is often attributed to the gravitational influence of an extended, non-spherical halo of proto-dark matter that permeates the volume defined by $R < 350 \text{ kpc}$ from the center of mass [4].
    Gravitational Parameter and Coupling