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Title: SEARCH FOR A CORRELATION BETWEEN ANTARES NEUTRINOS AND PIERRE AUGER OBSERVATORY UHECRs ARRIVAL DIRECTIONS

Journal Article · · Astrophysical Journal
; ;  [1]; ; ;  [2];  [3];  [4];  [5];  [6];  [7]; ; ; ;  [8]; ;  [9];  [10];  [11];  [12] more »; « less
  1. Institut d'Investigacio per a la Gestio Integrada de les Zones Costaneres (IGIC), Universitat Politecnica de Valencia, C/ Paranimf 1, E-46730 Gandia (Spain)
  2. CPPM, Aix-Marseille Universite, CNRS/IN2P3, F-13288 Marseille (France)
  3. GRPHE-Institut universitaire de technologie de Colmar, 34 rue du Grillenbreit BP 50568-68008 Colmar (France)
  4. Laboratory of Applied Bioacoustics, Technical University of Catalonia, Rambla Exposicio, E-08800 Vilanova i la Geltru, Barcelona (Spain)
  5. INFN-Sezione di Genova, Via Dodecaneso 33, I-16146 Genova (Italy)
  6. Friedrich-Alexander-Universitaet Erlangen-Nuernberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, D-91058 Erlangen (Germany)
  7. Direction des Sciences de la Matiere, Institut de recherche sur les lois fondamentales de l'Univers, Service d'Electronique des Detecteurs et d'Informatique, CEA Saclay, F-91191 Gif-sur-Yvette Cedex (France)
  8. Nikhef, Science Park, Amsterdam (Netherlands)
  9. APC-Laboratoire AstroParticule et Cosmologie, UMR 7164 (CNRS, Universite Paris 7 Diderot, CEA, Observatoire de Paris) 10, rue Alice Domon et Leonie Duquet, F-75205 Paris Cedex 13 (France)
  10. LAM-Laboratoire d'Astrophysique de Marseille, Pole de l'Etoile Site de Chateau-Gombert, rue Frederic Joliot-Curie 38, F-13388 Marseille Cedex 13 (France)
  11. INFN-Sezione di Bologna, Viale Berti-Pichat 6/2, I-40127 Bologna (Italy)
  12. IFIC-Instituto de Fisica Corpuscular, Edificios Investigacion de Paterna CSIC, Universitat de Valencia, Apdo. de Correos 22085, E-46071 Valencia (Spain)

A multimessenger analysis optimized for a correlation of arrival directions of ultra-high energy cosmic rays (UHECRs) and neutrinos is presented and applied to 2190 neutrino candidate events detected in 2007-2008 by the ANTARES telescope and 69 UHECRs observed by the Pierre Auger Observatory between 2004 January 1 and 2009 December 31. No significant correlation is observed. Assuming an equal neutrino flux (E {sup -2} energy spectrum) from all UHECR directions, a 90% CL upper limit on the neutrino flux of 5.0 Multiplication-Sign 10{sup -8} GeV cm{sup -2} s{sup -1} per source is derived.

OSTI ID:
22133977
Journal Information:
Astrophysical Journal, Vol. 774, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English