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Observational constraints of 30–40 GeV dark matter annihilation in galaxy clusters
Man Ho CHAN
Department of Science and Environmental Studies (SES)
Research output
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peer-review
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Dive into the research topics of 'Observational constraints of 30–40 GeV dark matter annihilation in galaxy clusters'. Together they form a unique fingerprint.
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Keyphrases
Dark Matter Annihilation
100%
Galaxy Clusters
100%
Observational Constraints
100%
Annihilation Cross Section
66%
Galactic Center
66%
Copyright
33%
Cosmic Rays
33%
Dark Matter
33%
Fermi-LAT
33%
Particle Dark Matter
33%
GeV γ-rays
33%
Profile Model
33%
Density Profile
33%
Gamma Rays
33%
Gamma-ray Spectrum
33%
Physics
Dark Matter
100%
Galaxy Clusters
100%
Gamma Radiation
66%
Galactic Center
66%