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Elsevier, Astroparticle Physics, (42), p. 7-14, 2013

DOI: 10.1016/j.astropartphys.2012.11.010

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Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles

Journal article published in 2013 by A. M. van den Berg, M. van der Hoek, S.; Institut d’Investigació per A. la Gestió integrada de les Zones Costaneres Universitat Politècnica València Gandia Spain Adrián-Martínez, M.; CPPM Aix-Marseille Université CNRS/IN2P3 France Ageron, V. van Beveren, J. A.; IFIC – Instituto de Física Corpuscular CSIC and Universitat de València Spain Aguilar, F.; Dublin Institute for Advanced Studies (DIAS) Ireland Aharonian, S.; Infn Sezione di Catania Italy Aiello, J.; IFIC – Instituto de Física Corpuscular CSIC and Universitat de València Spain Zúñiga, A.; Groupe de Recherche en Physique des Hautes Energies (GRPHE)/EA3438/Université de Haute Alsace Colmar France Albert, M.; Hellenic Centre for Marine Research (HCMR) Greece Alexandri, R. H. L. van Wooning, F.; Infn Sezione di Roma Italy Ameli, E. G.; University of Athens Greece Anassontzis, M.; Infn Sezione di Genova University of Italy Anghinolfi and other authors.
This paper is available in a repository.
This paper is available in a repository.

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Abstract

A recent analysis of the Fermi Large Area Telescope data provided evidence for a high-intensity emission of high-energy gamma rays with a E- 2 spectrum from two large areas, spanning 50º above and below the Galactic centre (the Fermi bubbles ). A hadronic mechanism was proposed for this gamma-ray emission making the Fermi bubbles promising source candidates of high-energy neutrino emission. In this work Monte Carlo simulations regarding the detectability of high-energy neutrinos from the Fermi bubbles with the future multi-km3 neutrino telescope KM3NeT in the Mediterranean Sea are presented. Under the hypothesis that the gamma-ray emission is completely due to hadronic processes, the results indicate that neutrinos from the bubbles could be discovered in about one year of operation, for a neutrino spectrum with a cutoff at 100 TeV and a detector with about 6 km3 of instrumented volume. The effect of a possible lower cutoff is also considered. ; European Community's Sixth Framework Programme [011937] ; Seventh Framework Programme [212525] ; S. Adrián-Martínez, M. Ageron, J.A. Aguilar et al. (2013). Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles. Astroparticle Physics. 42(1):7-14. doi:10.1016/j.astropartphys.2012.11.010. ; Senia ; 7 ; 14 ; 42 ; 1