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Isospin-violating dark matter at liquid noble detectors: new constraints, future projections, and an exploration of target complementarity

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arxiv 2302.05458 v2 pith:JAXPUBJM submitted 2023-02-10 hep-ph hep-ex

classification hep-phhep-ex
keywords modelstandardtargetargoncomplementarityconstraintsdarkdetectors
verification ladder T0 review T1 audit T2 compute T3 formal
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There is no known reason that dark matter interactions with the Standard Model should couple to neutrons and protons in the same way. This isospin violation can have large consequences, modifying the sensitivity of existing and future direct detection experimental constraints by orders of magnitude. Previous works in the literature have focused on the zero-momentum limit which has its limitations when extending the analysis to the Non-Relativistic Effective Field Theory basis (NREFT). In this paper, we study isospin violation in a detailed manner, paying specific attention to the experimental setups of liquid noble detectors. We analyse two effective Standard Model gauge invariant models as interesting case studies as well as the more model-independent NREFT operators. This work demonstrates the high degree of complementarity between the target nuclei xenon and argon. Most notably, we show that the Standard Model gauge-invariant formulation of the standard spin-dependent interaction often generates a sizeable response from argon, a target nuclei with zero spin. This work is meant as an update and a useful reference to model builders and experimentalists.

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Cited by 3 Pith papers

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

  1. $\texttt{SNuDD}$: Solar Neutrinos for Direct Detection

    hep-ph 2026-07 conditional novelty 5.0 of 10

    SNuDD computes solar-neutrino recoil spectra with non-standard interactions and derives NSI limits from xenon direct-detection data that are competitive with dedicated neutrino experiments.

  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...

  3. Neutrino fog in the light dark sector: the role of isospin violation

    hep-ph 2025-08 unverdicted novelty 5.0 of 10

    In a U(1)' dark sector model, isospin-violating couplings shift both the neutrino floor and the DM exclusion bound, changing the window for light dark matter discovery.

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