A Dark Matter Candidate with New Strong Interactions
arXiv:hep-ph/0506015 · doi:10.1103/PhysRevD.72.043530
Abstract
We study the possibility that dark matter is a baryon of a new strongly interacting gauge theory, which was introduced in the low energy theory of Cosmological SUSY Breaking (CSB). This particle can fit the observed dark matter density if an appropriate cosmological asymmetry is generated. The same mechanism can also explain the dark/baryonic matter ratio in the universe. The mass of the dark matter particle is in the multiple TeV range, and could be as high as 20 TeV.
Revised to include a disclaimer in paragraph 3 of page 5. Typo removed in equation for angular momentum of soliton-anti-soliton scattering, in paragraph 3 of section 2
References in corpus (5)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Dark Matter Profile in the Galactic Center
- Detecting Technibaryon Dark Matter
- TeV -radiation from Dark Matter annihilation in the Galactic center
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- Collider Constraints on Dipole-Interacting Dark Matter
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- Superheavy Thermal Dark Matter and Primordial Asymmetries
- Composite bosonic baryon dark matter on the lattice: SU(4) baryon spectrum and the effective Higgs interaction
- WIMPless Dark Matter from Non-Abelian Hidden Sectors with Anomaly-Mediated Supersymmetry Breaking
- Cosmic Ray-Dark Matter Scattering: a New Signature of (Asymmetric) Dark Matter in the Gamma Ray Sky
- Holographic space-time and its phenomenological implications
- Dark Matter Model or Mass, but Not Both: Assessing Near-Future Direct Searches with Benchmark-free Forecasting
- A Pyramid Scheme for Particle Physics
- Color-flavor locked strangelets in a quark mass density-dependent model
- Update on the Pyramid Scheme
- Cosmological SUSY Breaking and the Pyramid Schemes