Asymmetric dark matter and the hadronic spectra of hidden QCD

Stephen J. Lonsdale, Martine Schroor, and Raymond R. Volkas
Phys. Rev. D 96, 055027 – Published 18 September 2017

Abstract

The idea that dark matter may be a composite state of a hidden non-Abelian 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×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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  • Received 29 May 2017

DOI:https://doi.org/10.1103/PhysRevD.96.055027

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsGravitation, Cosmology & Astrophysics

Authors & Affiliations

Stephen J. Lonsdale1,*, Martine Schroor2, and Raymond R. Volkas1

  • 1ARC Centre of Excellence for Particle Physics at the Terascale, School of Physics, The University of Melbourne, Victoria 3010, Australia
  • 2Van Swinderen Institute for Particle Physics and Gravity, University of Groningen, Nijenborgh 4, 9747 AG Groningen, The Netherlands

  • *lsj@student.unimelb.edu.au

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Issue

Vol. 96, Iss. 5 — 1 September 2017

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