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Asymmetric Dark Matter and the hadronic spectra of hidden QCD

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arxiv 1704.05213 v2 pith:Z2XDB5DW submitted 2017-04-18 hep-ph

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

The idea that dark matter may be a composite state of a hidden nonabelian gauge sector has received great attention in recent years. Frameworks such as asymmetric dark matter motivate the idea that dark matter may have similar mass to the proton, while mirror matter and $G \times G$ grand unified theories provide rationales for additional gauge sectors which may have minimal interactions with standard model particles. In this work we explore the hadronic spectra that these dark QCD models can allow. The effects of the number of light colored particles and the value of the confinement scale on the lightest stable state, the dark matter candidate, are examined in the hyperspherical constituent quark model for baryonic and mesonic states.

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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. Composite asymmetric dark matter with a dark photon portal: Multimessenger tests

    hep-ph 2024-12 conditional novelty 6.0 of 10

    Decaying composite dark matter in the 1 to 10 GeV mass range is most strongly constrained by AMS-02 positron data, needing lifetimes above roughly 10^26 seconds.

  2. Direct Detection and Cosmological Constraints of Dark Matter with Dark Dipoles

    hep-ph 2026-02 conditional novelty 5.0 of 10

    Cosmological and direct-detection data already exclude most sub-GeV dark-matter parameter space for dark-photon magnetic dipole interactions, with semiconductor detectors needed to probe the remaining electric-dipole ...

  3. Rich Phenomenology from Simple Ingredients: A Review of Confining Dark Sectors

    hep-ph 2026-06 unverdicted novelty 2.0 of 10

    Review of confining dark sectors summarizing dark matter candidates, abundance mechanisms, discovery channels, and applications to the abundance similarity puzzle.

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