Skip to main navigation Skip to search Skip to main content

Search for Dark Matter Annihilation Signals in the H.E.S.S. Inner Galaxy Survey

  • (H.E.S.S. Collaboration)
  • University of Namibia
  • Dublin Institute for Advanced Studies
  • Max-Planck-Institut für Kernphysik
  • Russian-Armenian University
  • Aix Marseille Université
  • Université Savoie Mont Blanc
  • Université Paris-Saclay
  • North-West University
  • Institute for Nuclear Physics
  • c/o DESY
  • University of the Witwatersrand, Johannesburg
  • Linnaeus University, Växjö
  • University of Tübingen
  • Sorbonne Université
  • Laboratoire de Probabilités et Modèles Aléatoires
  • University of Oxford
  • Univ. Bordeaux
  • LUTH - Laboratoire de l'Univers et de ses Theories
  • University of Potsdam
  • Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
  • University of Innsbruck
  • Universität Hamburg
  • Jagiellonian University
  • Landessternwarte Heidelberg
  • Nicolaus Copernicus University
  • Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
  • Humboldt-Universität zu Berlin
  • Laboratoire Univers et Particules de Montpellier
  • University of Adelaide
  • Yerevan Physics Institute
  • University of Tokyo
  • Konan University
  • Riken
  • Rikkyo University
  • University of Amsterdam

Research output: Contribution to journalArticlepeer-review

101 Citations (Scopus)

Abstract

The central region of the Milky Way is one of the foremost locations to look for dark matter (DM) signatures. We report the first results on a search for DM particle annihilation signals using new observations from an unprecedented γ-ray survey of the Galactic Center (GC) region, i.e., the Inner Galaxy Survey, at very high energies (?100 GeV) performed with the H.E.S.S. array of five ground-based Cherenkov telescopes.

Original languageEnglish
Article number111101
JournalPhysical Review Letters
Volume129
Issue number11
DOIs
Publication statusPublished - 9 Sept 2022
Externally publishedYes

Fingerprint

Dive into the research topics of 'Search for Dark Matter Annihilation Signals in the H.E.S.S. Inner Galaxy Survey'. Together they form a unique fingerprint.

Cite this