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Journal Article | PUBDB-2023-05032 |
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2023
APS
College Park, Md.
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Please use a persistent id in citations: doi:10.1103/PhysRevLett.130.061002 doi:10.3204/PUBDB-2023-05032
Report No.: KEK-Cosmo-0307; KEK-TH-2487; arXiv:2212.10527
Abstract: Linelike features in TeV γ rays constitute a “smoking gun” for TeV-scale particle dark matter and new physics. Probing the Galactic Center region with ground-based Cherenkov telescopes enables the search for TeV spectral features in immediate association with a dense dark matter reservoir at a sensitivity out of reach for satellite γ-ray detectors, and direct detection and collider experiments. We report on 223 hours of observations of the Galactic Center region with the MAGIC stereoscopic telescope system reaching γ-ray energies up to 100 TeV. We improved the sensitivity to spectral lines at high energies using large-zenith-angle observations and a novel background modeling method within a maximum-likelihood analysis in the energy domain. No linelike spectral feature is found in our analysis. Therefore, we constrain the cross section for dark matter annihilation into two photons to ⟨σv⟩≲5×10-28 cm3 s-1 at 1 TeV and ⟨σv⟩≲1×10-25 cm3 s-1 at 100 TeV, achieving the best limits to date for a dark matter mass above 20 TeV and a cuspy dark matter profile at the Galactic Center. Finally, we use the derived limits for both cuspy and cored dark matter profiles to constrain supersymmetric wino models.
Keyword(s): dark matter: annihilation ; energy: high ; dark matter: mass ; scale: TeV ; up: annihilation ; spectral ; galaxy ; MAGIC ; sensitivity ; satellite ; direct detection ; two-photon ; background ; new physics ; Cherenkov counter ; supersymmetry ; gamma ray
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Search for Gamma-ray Spectral Lines from Dark Matter Annihilation up to 100 TeV towards the Galactic Center with MAGIC
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