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  1. Cold Dark Matter (cdm)

    Linked via "WIMP"

    Direct Detection Experiments
    These facilities, such as LUX-ZEPLIN (LZ)) and XENONnT, search for the tiny nuclear recoil energy ($\approx 1-100 \text{ keV}$) generated by a WIMP impact. Current limits have excluded large regions of the WIMP parameter space defined by the minimal Supersymmetric Standard Model (MSSM)) [5].
    Indirect Detection Experiments

  2. Cold Dark Matter (cdm)

    Linked via "WIMP"

    Indirect Detection Experiments
    Indirect detection focuses on looking for the decay or annihilation products of CDM) in regions of high dark matter density, such as the Galactic Center or dwarf spheroidal galaxies. If CDM) particles annihilate, they should produce detectable high-energy Standard Model particles, particularly gamma rays, neutrinos, or [antim…