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Shifting the neutrino fog: studying the Isospin-violating Dark Matter case

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arxiv 2512.19784 v2 pith:R6OPNA7A submitted 2025-12-22 hep-ph

Shifting the neutrino fog: studying the Isospin-violating Dark Matter case

classification hep-ph
keywords neutrinomodelsdarkmatterbackgroundcaseisospin-violatingivdm
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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First observation of solar neutrinos through coherent elastic neutrino-nucleus scattering by dark matter (DM) direct detection (DD) experiments makes the study of the neutrino fog of the most relevance. This irreducible neutrino background depends on the target material as well as other experimental parameters. Recently, it has also been remarked the dependence of the neutrino fog on the DM models under consideration. In this work, we study the case of Isospin-violating dark matter (IVDM) models, discussing specific examples of DM models and making a detailed analysis of the implications of IVDM on the neutrino fog. We also explore the conditions under which this background can be mitigated for specific DM models.

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Cited by 1 Pith paper

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  1. Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering

    hep-ph 2026-05 unverdicted novelty 4.0

    Future dark matter detectors with ~3000 ton-yr exposure could probe sterile neutrino mixing with νμ and ντ in parameter space not reached by long-baseline or atmospheric searches.