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Hadronic and hadron-like physics of Dark Matter

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arxiv 1904.12013 v1 pith:SEDDWAKF submitted 2019-04-26 hep-ph

Hadronic and hadron-like physics of Dark Matter

classification hep-ph
keywords darkmatterparticlesphysicscandidateselementaryacceleratorappeal
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The problems of simple elementary weakly interacting massive particles (WIMPs) appeal to extend the physical basis for nonbaryonic dark matter. Such extension involves more sophisticated dark matter candidates from physics beyond the Standard Model (BSM) of elementary particles. We discuss several models of dark matter, predicting new colored, hyper-colored or techni-colored particles and their accelerator and non-accelerator probes. The nontrivial properties of the proposed dark matter candidates can shed new light on the dark matter physics. They provide interesting solutions for the puzzles of direct and indirect dark matter search.

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Cited by 2 Pith papers

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

  1. Finite-temperature Yang-Mills theories with the density of states method: towards the continuum limit

    hep-lat 2025-09 unverdicted novelty 5.0

    Density-of-states lattice study of the first-order phase transition in Sp(4) Yang-Mills theory at finite temperature, confirming metastability and surface tension for two temporal extents toward the continuum limit.

  2. Formation of Asymmetrical Two-Brane Structure and its Possible Manifestation

    hep-th 2025-02 unverdicted novelty 3.0

    In a two-brane model, brane asymmetry produces different fermion masses, allowing superheavy leptons on the second brane to act as dark matter without fine-tuning.