Search for gamma-ray spectral lines from dark matter annihilation with the H.E.S.S. Inner Galaxy Survey
astro-ph.HE
Submitted: 2026-08-07
Updated: 2026-08-07
Comments: Accepted in Phys. Rev. Lett., includes Supplemental materials. 6+7 pages, 2+1 figures, 0+2 tables
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- Non-Baryonic Dark Matter - Observational Evidence and Detection Methods
- Supersymmetric Dark Matter
- Minimal Dark Matter
- Cosmology and Astrophysics of Minimal Dark Matter
- Minimal Dark Matter predictions for galactic positrons, anti-protons, photons
- Minimal Dark Matter: model and results
- Gamma ray tests of Minimal Dark Matter
- The Minimal Model for Dark Matter and Unification
- $Z$ boson mediated dark matter beyond the effective theory
- Direct Detection of WIMP Dark Matter: Concepts and Status
- Review of LHC Dark Matter Searches
- Closing the window on WIMP Dark Matter
- The last Complex WIMPs standing
- Hunting wino and higgsino dark matter at the muon collider with disappearing tracks
- Discovery reach for wino and higgsino dark matter with a disappearing track signature at a 100 TeV $pp$ collider
- Universal behavior in the scattering of heavy, weakly interacting dark matter on nuclear targets
- WIMP-nucleon scattering with heavy WIMP effective theory
- Standard Model anatomy of WIMP dark matter direct detection I: weak-scale matching
- QCD Effects on Direct Detection of Wino Dark Matter
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