Constraints on dark matter annihilation in clusters of galaxies from diffuse radio emission

Keyphrases

• Galaxy Clusters 100%
• Diffuse Radio Emission 100%
• Dark Matter Annihilation 100%
• Dark Matter 66%
• Substructure Model 66%
• Mini 33%
• Radio Emission 33%
• Radio 33%
• Synchrotron Radiation 33%
• Magnetic Field 33%
• Substructure 33%
• Halo 33%
• Phoenix Project 33%
• Magnetic Field Structure 33%
• Gamma Rays 33%
• Order of Magnitude 33%
• Model Particle 33%
• Annihilation Cross Section 33%
• Channel Model 33%
• Non-detection 33%
• Positron 33%
• Diffuse Emission 33%
• Derived Limit 33%
• Case Cluster 33%
• Strong Limit 33%
• Dark Matter Mass 33%

Physics

• Galaxy Clusters 100%
• Radio Emission 100%
• Dark Matter 100%
• Magnetic Field 33%
• Gamma Radiation 16%
• Standard Model 16%
• Positron 16%
• Navarro-Frenk-White Profile 16%
• Synchrotron Radiation 16%