Electroweak Doublet Dark Matter for a Galactic Halo Gamma-Ray Excess
hep-ph, astro-ph.CO
Submitted: 2026-04-06
Updated: 2026-08-31
Comments: 5 pages, 1 figure
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation
- 20 GeV halo-like excess of the Galactic diffuse emission and implications for dark matter annihilation
- The Characterization of the Gamma-Ray Signal from the Central Milky Way: A Compelling Case for Annihilating Dark Matter
- The Fermi Galactic Center GeV Excess and Implications for Dark Matter
- Improved Naturalness with a Heavy Higgs: An Alternative Road to LHC Physics
- Inelastic Dark Matter
- Dark Matter implications from the LZ, PandaX-4T and XENONnT Data
- First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
- First Dark Matter Search with Nuclear Recoils from the XENONnT Experiment
- Relic density of Dark Matter in the Inert Doublet Model beyond Leading Order. I) The Heavy Mass Case
- Constraints on the Inert Doublet Model of dark matter with very high-energy gamma-ray observatories
- Non-Perturbative Effect on Dark Matter Annihilation and Gamma Ray Signature from Galactic Center
- Legacy Analysis of Dark Matter Annihilation from the Milky Way Dwarf Spheroidal Galaxies with 14 Years of Fermi-LAT Data
- Resonant Annihilation of WIMP Dark Matter for Halo Gamma Ray Signal
- Aspects of Sommerfeld Enhancement in the light of Halo gamma-ray excess
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