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Direct detection of light dark matter charged under a $L_{\mu} - L_{\tau}$ symmetry

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arxiv 2404.03090 v2 pith:7ZEEBLL6 submitted 2024-04-03 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords darkmattersymmetrychargedunderableanomalousdetection
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

A possible extension of the Standard Model able to explain the recent measurement of the anomalous magnetic moment of the muon consists in adding a gauged $U(1)_{L_{\mu}-L_{\tau}}$ symmetry. If the dark matter particle is charged under this symmetry, the kinetic mixing between the new gauge boson and the photon induces dark matter-electron interactions. We derive direct detection constraints on light dark matter charged under a $U(1)_{L_{\mu}-L_{\tau}}$ symmetry with electron recoil experiments, and explore prospects with XLZD and OSCURA to close in the parameter space able to explain simultaneously the recent measurement on the anomalous magnetic moment of the muon and the observed relic density of dark matter. We further discuss the spin-dependent scattering contribution arising in this model, which was ignored previously in the literature.

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

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    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...

  2. Sub-GeV Dark Matter Under Pressure from Direct Detection

    hep-ph 2025-07 conditional novelty 4.0 of 10

    PandaX-4T S2-only data yields world-leading sub-GeV dark matter-electron scattering limits for heavy mediators in the 20-200 MeV range, although the result largely overlaps with the collaboration's own just-released analysis.

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