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Determining Spin-Dependent Light Dark Matter Rates from Neutron Scattering

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arxiv 2504.02927 v2 pith:BCKQ3KLZ submitted 2025-04-03 hep-ph astro-ph.COcond-mat.mtrl-scicond-mat.str-elhep-ex

classification hep-phastro-ph.COcond-mat.mtrl-scicond-mat.str-elhep-ex
keywords darkmatterscatteringtargetneutronexperimentslightmasses
verification ladder T0 review T1 audit T2 compute T3 formal
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The scattering and absorption rates of light dark matter with electron spin-dependent interactions depend on the target's spin response. We show how this response is encoded by the target's dynamical magnetic susceptibility, which can be measured using neutron scattering. We directly use existing neutron scattering data to compute the dark matter scattering rate in a candidate target material, finding close agreement with the previous first-principles calculation at MeV dark matter masses. Complementary experiments and measurements can extend the reach of this technique to other dark matter models and masses, and identify promising target materials for future experiments.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Spin-Dependent Scattering of Sub-GeV Dark Matter: Models and Constraints

    hep-ph 2025-06 conditional novelty 8.0 of 10

    A new calculation of spin-dependent sub-GeV dark matter phonon scattering shows only the light scalar mediator model retains testable parameter space, conditional on the supernova trapping window.

  2. 2024 TASI Lectures: A Dark Matter Primer

    hep-ph 2025-06 conditional novelty 1.0 of 10

    A graduate-level primer covering the evidence for dark matter, the main cosmological production mechanisms (freeze-out, freeze-in, misalignment), and the direct detection formalism, with no new results.

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