Decaying Dark Matter Baryons in a Composite Messenger Model
arXiv:0811.0737 · doi:10.1016/j.physletb.2009.03.025
Abstract
A baryonic bound state with a mass of O(100) TeV, which is composed of strongly interacting messenger quarks in the low scale gauge mediation, can naturally be the cold dark matter. Interestingly, we find that such a baryonic dark matter is generically metastable, and the decay of this dark matter can naturally explain the anomalous positron flux recently observed by the PAMELA collaboration.
10 pages, 2 figures. v2: minor changes, note added
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- Gamma rays and positrons from a decaying hidden gauge boson
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Cited by in corpus (50)
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- Constraining Very Heavy Dark Matter Using Diffuse Backgrounds of Neutrinos and Cascaded Gamma Rays
- Indirect Searches for Decaying Dark Matter
- Phenomenology of charged dark matter at PAMELA/FERMI and colliders
- Excesses in the Cosmic Ray Spectrum and Possible Interpretations
- Cosmic Signals from the Hidden Sector
- Discriminating different scenarios to account for the cosmic excess by synchrotron and inverse Compton radiation
- Parameters in a Class of Leptophilic Dark Matter Models from PAMELA, ATIC and FERMI
- White Dwarf Pulsars as Possible Cosmic Ray Electron-Positron Factories
- Cosmic Ray Positron and Electron Excess from Hidden-Fermion Dark Matter Decays
- Precise WIMP Dark Matter Abundance and Standard Model Thermodynamics
- Radio and gamma-ray constraints on dark matter annihilation in the Galactic center
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- Secondary radiation from the Pamela/ATIC excess and relevance for Fermi
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- Synchrotron Radiation from the Galactic Center in Decaying Dark Matter Scenario
- Annihilation vs. Decay: Constraining dark matter properties from a gamma-ray detection
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- Galactic Signatures of Decaying Dark Matter
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- Multicomponent Dark Matter in the Light of CALET and DAMPE