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Exploring properties of long-lived particles in inelastic dark matter models at Belle II

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arxiv 2101.02503 v2 pith:VAGPHUI7 submitted 2021-01-07 hep-ph hep-ex

classification hep-phhep-ex
keywords darkmassbelleexcitedmatterdisplacedinelasticmodels
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

The inelastic dark matter model is one kind of popular models for the light dark matter (DM) below $O(1)$ GeV. If the mass splitting between DM excited and ground states is small enough, the co-annihilation becomes the dominant channel for thermal relic density and the DM excited state can be long-lived at the collider scale. We study scalar and fermion inelastic dark matter models for $ {\cal O}(1) $ GeV DM at Belle II with $ U(1)_D $ dark gauge symmetry broken into its $Z_2$ subgroup. We focus on dilepton displaced vertex signatures from decays of the DM excited state. With the help of precise displaced vertex detection ability at Belle II, we can explore the DM spin, mass and mass splitting between DM excited and ground states. Especially, we show scalar and fermion DM candidates can be discriminated and the mass and mass splitting of DM sector can be determined within the percentage of deviation for some benchmark points. Furthermore, the allowed parameter space to explain the excess of muon $(g-2)_\mu$ is also studied and it can be covered in our displaced vertex analysis during the early stage of Belle II experiment.

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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. Estimating the track-reconstruction efficiency in phenomenological proposals of long-lived-particle searches

    hep-ex 2025-01 conditional novelty 6.0 of 10

    TrackEff estimates Belle II track-reconstruction efficiency by geometrically counting drift-chamber hits, with default thresholds tuned to a Belle II tau-tau tracking efficiency measurement.

  2. 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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