Gamma-Ray Excess and the Minimal Dark Matter Model
arXiv:1510.07562 · doi:10.1007/JHEP06(2016)008
Abstract
We point out that the gamma-ray excesses in the galactic center and in the dwarf galaxy Reticulum II can both be well explained within the simplest dark matter model. We find that the corresponding region of parameter space will be tested by direct and indirect dark matter searches in the near future.
6 pages, 8 figures; v2: new LUX bounds included, to appear in JHEP
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Cited by in corpus (16)
- Reopening the Higgs portal for Singlet Scalar Dark Matter
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- Dark Matter meets Quantum Gravity
- Probing dark matter annihilation in the Galaxy with antiprotons and gamma rays
- Minimal conformal extensions of the Higgs sector
- Model-independent analysis of the DAMPE excess
- A global fit of the -ray galactic center excess within the scalar singlet Higgs portal model
- New LUX and PandaX-II Results Illuminating the Simplest Higgs-Portal Dark Matter Models
- Improved bounds on singlet dark matter
- GAMBIT and its Application in the Search for Physics Beyond the Standard Model
- A Closer Look at CP-Violating Higgs Portal Dark Matter as a Candidate for the GCE
- The Galactic Center Excess from Z3 Scalar Semi-Annihilations
- Gamma Lines from the Hidden Sector
- Phenomenology of Colored Radiative Neutrino Mass Model and Its Implications on the Cosmic-ray Observations
- Extended Higgs-portal dark matter and the Fermi-LAT Galactic Center Excess
- Dark matter properties implied by gamma ray interstellar emission models