Physics Letters B (Jun 2017)

Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope

  • A. Albert,
  • M. André,
  • M. Anghinolfi,
  • G. Anton,
  • M. Ardid,
  • J.-J. Aubert,
  • T. Avgitas,
  • B. Baret,
  • J. Barrios-Martí,
  • S. Basa,
  • V. Bertin,
  • S. Biagi,
  • R. Bormuth,
  • S. Bourret,
  • M.C. Bouwhuis,
  • R. Bruijn,
  • J. Brunner,
  • J. Busto,
  • A. Capone,
  • L. Caramete,
  • J. Carr,
  • S. Celli,
  • T. Chiarusi,
  • M. Circella,
  • J.A.B. Coelho,
  • A. Coleiro,
  • R. Coniglione,
  • H. Costantini,
  • P. Coyle,
  • A. Creusot,
  • A. Deschamps,
  • G. De Bonis,
  • C. Distefano,
  • I. Di Palma,
  • C. Donzaud,
  • D. Dornic,
  • D. Drouhin,
  • T. Eberl,
  • I. El Bojaddaini,
  • D. Elsässer,
  • A. Enzenhöfer,
  • I. Felis,
  • L.A. Fusco,
  • S. Galatà,
  • P. Gay,
  • S. Geißelsöder,
  • K. Geyer,
  • V. Giordano,
  • A. Gleixner,
  • H. Glotin,
  • T. Grégoire,
  • R. Gracia Ruiz,
  • K. Graf,
  • S. Hallmann,
  • H. van Haren,
  • A.J. Heijboer,
  • Y. Hello,
  • J.J. Hernández-Rey,
  • J. Hößl,
  • J. Hofestädt,
  • C. Hugon,
  • G. Illuminati,
  • C.W. James,
  • M. de Jong,
  • M. Jongen,
  • M. Kadler,
  • O. Kalekin,
  • U. Katz,
  • D. Kießling,
  • A. Kouchner,
  • M. Kreter,
  • I. Kreykenbohm,
  • V. Kulikovskiy,
  • C. Lachaud,
  • R. Lahmann,
  • D. Lefèvre,
  • E. Leonora,
  • M. Lotze,
  • S. Loucatos,
  • M. Marcelin,
  • A. Margiotta,
  • A. Marinelli,
  • J.A. Martínez-Mora,
  • A. Mathieu,
  • R. Mele,
  • K. Melis,
  • T. Michael,
  • P. Migliozzi,
  • A. Moussa,
  • C. Mueller,
  • E. Nezri,
  • G.E. Păvălaş,
  • C. Pellegrino,
  • C. Perrina,
  • P. Piattelli,
  • V. Popa,
  • T. Pradier,
  • L. Quinn,
  • C. Racca,
  • G. Riccobene,
  • K. Roensch,
  • A. Sánchez-Losa,
  • M. Saldaña,
  • I. Salvadori,
  • D.F.E. Samtleben,
  • M. Sanguineti,
  • P. Sapienza,
  • J. Schnabel,
  • F. Schüssler,
  • T. Seitz,
  • C. Sieger,
  • M. Spurio,
  • Th. Stolarczyk,
  • M. Taiuti,
  • Y. Tayalati,
  • A. Trovato,
  • M. Tselengidou,
  • D. Turpin,
  • C. Tönnis,
  • B. Vallage,
  • C. Vallée,
  • V. Van Elewyck,
  • D. Vivolo,
  • A. Vizzoca,
  • S. Wagner,
  • J. Wilms,
  • J.D. Zornoza,
  • J. Zúñiga

DOI
https://doi.org/10.1016/j.physletb.2017.03.063
Journal volume & issue
Vol. 769, no. C
pp. 249 – 254

Abstract

Read online

Using data recorded with the ANTARES telescope from 2007 to 2015, a new search for dark matter annihilation in the Milky Way has been performed. Three halo models and five annihilation channels, WIMP+WIMP→bb¯,W+W−,τ+τ−,μ+μ− and νν¯, with WIMP masses ranging from 50 GeVc2 to 100 TeVc2, were considered. No excess over the expected background was found, and limits on the thermally averaged annihilation cross-section were set.

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