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$Z$ boson mediated dark matter beyond the effective theory

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arxiv 1611.05048 v2 pith:AYMKQQG7 submitted 2016-11-15 hep-ph

classification hep-ph
keywords modeldarkbosondetectiondirectmattermediatedparameter
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

Direct detection bounds are beginning to constrain a very simple model of weakly interacting dark matter---a Majorana fermion with a coupling to the $Z$ boson. In a particularly straightforward gauge-invariant realization, this coupling is introduced via a higher-dimensional operator. While attractive in its simplicity, this model generically induces a large $\rho$ parameter. An ultraviolet completion that avoids an overly large contribution to $\rho$ is the singlet-doublet model. We revisit this model, focusing on the Higgs blind spot region of parameter space where spin-independent interactions are absent. This model successfully reproduces dark matter with direct detection mediated by the $Z$ boson, but whose cosmology may depend on additional couplings and states. Future direct detection experiments should effectively probe a significant portion of this parameter space, aside from a small coannihilating region. As such, $Z$-mediated thermal dark matter as realized in the singlet-doublet model represents an interesting target for future searches.

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Cited by 3 Pith papers

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

  1. Singlet-doublet dark matter beyond freeze-out

    hep-ph 2026-08 conditional novelty 6.0 of 10

    In the small-coupling limit of the singlet-doublet dark matter model, the relic density is set by co-scattering, freeze-in, or SuperWIMP decays rather than ordinary freeze-out, and the observable signals move from dir...

  2. Singlet-doublet dark matter revisited

    hep-ph 2025-05 conditional novelty 5.0 of 10

    The singlet-doublet dark matter model now passes direct detection limits only with small Yukawa couplings or near blind spots, with coannihilation and a compressed spectrum needed to match the observed relic density.

  3. Dark Photon mediated Inelastic Dark Matter in Cosmology, Astrophysics and Colliders

    hep-ph 2026-02 conditional novelty 4.0 of 10

    Full relic-density-allowed parameter space of dark-photon inelastic dark matter is mapped at α_D=α_EM, with FASER sensitive up to Mχ1≈7 GeV and neutron-star heating up to ~2000 K.

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