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The role of ionization electrons in direct dark matter detection

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arxiv hep-ph/0401151 v3 pith:KGPWCADD submitted 2004-01-21 hep-ph

J.D. Vergados (University of Cyprus , Nicosia , Cyprus) , H.Ejiri (Emeritus , RCNP , Osaka , Japan) This is my paper · ORCID
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keywords electronsenergyestimateionizationneutralinoscatteringthresholdaround
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In this paper we estimate the event rates of neutralino-nucleus scattering leading to electron emission by the atomic ionization. We find that the branching ratio for detecting electrons vis a vis the traditional neutralino nucleus elastic scattering sensitively depends on the threshold energy. In the case of a light target and a neutralino mass of 100 GeV we estimate it to be around 10 percent assuming a reasonable threshold energy of 250 eV.

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  1. Migdal Ionization as a Probe of Light Dark Matter from Nuclear Transition

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Migdal ionization of reactor-produced sub-MeV dark matter in TEXONO germanium yields new 95% C.L. limits on the reference DM–proton cross section for 0.01 MeV ≤ mχ ≲ 2.6 MeV.

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