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The Non-Relativistic Effective Field Theory Of Dark Matter-Electron Interactions

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arxiv 2407.14598 v2 pith:CEQLB6CJ submitted 2024-07-19 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords dm-electronelectroninteractionsdarkgeneralhigh-energylightderive
verification ladder T0 review T1 audit T2 compute T3 formal
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Electronic excitations in atomic, molecular, and crystal targets are at the forefront of the ongoing search for light, sub-GeV dark matter (DM). In many light DM-electron interactions the energy and momentum deposited is much smaller than the electron mass, motivating a non-relativistic (NR) description of the electron. Thus, for any target, light DM-electron phenomenology relies on understanding the interactions between the DM and electron in the NR limit. In this work we derive the NR effective field theory (EFT) of general DM-electron interactions from a top-down perspective, starting from general high-energy DM-electron interaction Lagrangians. This provides an explicit connection between high-energy theories and their low-energy phenomenology in electron excitation based experiments. Furthermore, we derive Feynman rules for the DM-electron NR EFT, allowing observables to be computed diagrammatically, which can systematically explain the presence of in-medium screening effects in general DM models. We use these Feynman rules to compute absorption, scattering, and dark Thomson scattering rates for a wide variety of high-energy DM models.

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Cited by 2 Pith papers

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  1. First-principles upper bounds on dark matter-electron scattering rates from condensed matter sum rules

    hep-ph 2026-08 conditional novelty 6.0 of 10

    Dark matter-electron scattering rates in isotropic materials are bounded from above by a universal expression depending only on plasma frequency, mass density, and static dielectric function.

  2. Information-theoretic astrophysical uncertainties in the effective theory of dark matter direct detection

    hep-ph 2026-01 conditional novelty 5.0 of 10

    Using an information-theoretic bound on the halo velocity distribution, dark matter direct-detection limits vary from <10x to ~10,000x near threshold depending on the EFT operator, with higher velocity-weighting opera...

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