@article{3073351, title = "Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles", author = "Adrián-Martínez, S. and Ageron, M. and Aguilar, J.A. and Aharonian, F. and Aiello, S. and Albert, A. and Alexandri, M. and Ameli, F. and Anassontzis, E.G. and Anghinolfi, M. and Anton, G. and Anvar, S. and Ardid, M. and Assis Jesus, A. and Aubert, J.-J. and Bakker, R. and Ball, A.E. and Barbarino, G. and Barbarito, E. and Barbato, F. and Baret, B. and De Bel, M. and Belias, A. and Bellou, N. and Berbee, E. and Berkien, A. and Bersani, A. and Bertin, V. and Beurthey, S. and Biagi, S. and Bigongiari, C. and Bigourdan, B. and Billault, M. and De Boer, R. and Boer Rookhuizen, H. and Bonori, M. and Borghini, M. and Bou-Cabo, M. and Bouhadef, B. and Bourlis, G. and Bouwhuis, M. and Bradbury, S. and Brown, A. and Bruni, F. and Brunner, J. and Brunoldi, M. and Busto, J. and Cacopardo, G. and Caillat, L. and Calvo Díaz-Aldagalán, D. and Calzas, A. and Canals, M. and Capone, A. and Carr, J. and Castorina, E. and Cecchini, S. and Ceres, A. and Cereseto, R. and Chaleil, T. and Chateau, F. and Chiarusi, T. and Choqueuse, D. and Christopoulou, P.E. and Chronis, G. and Ciaffoni, O. and Circella, M. and Cocimano, R. and Cohen, F. and Colijn, F. and Coniglione, R. and Cordelli, M. and Cosquer, A. and Costa, M. and Coyle, P. and Craig, J. and Creusot, A. and Curtil, C. and D'Amico, A. and Damy, G. and De Asmundis, R. and De Bonis, G. and Decock, G. and Decowski, P. and Delagnes, E. and De Rosa, G. and Distefano, C. and Donzaud, C. and Dornic, D. and Dorosti-Hasankiadeh, Q. and Drogou, J. and Drouhin, D. and Druillole, F. and Drury, L. and Durand, D. and Durand, G.A. and Eberl, T. and Emanuele, U. and Enzenhöfer, A. and Ernenwein, J.-P. and Escoffier, S. and Espinosa, V. and Etiope, G. and Favali, P. and Felea, D. and Ferri, M. and Ferry, S. and Flaminio, V. and Folger, F. and Fotiou, A. and Fritsch, U. and Gajanana, D. and Garaguso, R. and Gasparini, G.P. and Gasparoni, F. and Gautard, V. and Gensolen, F. and Geyer, K. and Giacomelli, G. and Gialas, I. and Giordano, V. and Giraud, J. and Gizani, N. and Gleixner, A. and Gojak, C. and Gómez-González, J.P. and Graf, K. and Grasso, D. and Grimaldi, A. and Groenewegen, R. and Guédé, Z. and Guillard, G. and Guilloux, F. and Habel, R. and Hallewell, G. and Van Haren, H. and Van Heerwaarden, J. and Heijboer, A. and Heine, E. and Hernández-Rey, J.J. and Herold, B. and Hillebrand, T. and Van De Hoek, M. and Hogenbirk, J. and Hößl, J. and Hsu, C.C. and Imbesi, M. and Jamieson, A. and Jansweijer, P. and De Jong, M. and Jouvenot, F. and Kadler, M. and Kalantar-Nayestanaki, N. and Kalekin, O. and Kappes, A. and Karolak, M. and Katz, U.F. and Kavatsyuk, O. and Keller, P. and Kiskiras, Y. and Klein, R. and Kok, H. and Kontoyiannis, H. and Kooijman, P. and Koopstra, J. and Kopper, C. and Korporaal, A. and Koske, P. and Kouchner, A. and Koutsoukos, S. and Kreykenbohm, I. and Kulikovskiy, V. and Laan, M. and La Fratta, C. and Lagier, P. and Lahmann, R. and Lamare, P. and Larosa, G. and Lattuada, D. and Leisos, A. and Lenis, D. and Leonora, E. and Le Provost, H. and Lim, G. and Llorens, C.D. and Lloret, J. and Löhner, H. and Lo Presti, D. and Lotrus, P. and Louis, F. and Lucarelli, F. and Lykousis, V. and Malyshev, D. and Mangano, S. and Marcoulaki, E.C. and Margiotta, A. and Marinaro, G. and Marinelli, A. and Mariş, O. and Markopoulos, E. and Markou, C. and Martínez-Mora, J.A. and Martini, A. and Marvaldi, J. and Masullo, R. and Maurin, G. and Migliozzi, P. and Migneco, E. and Minutoli, S. and Miraglia, A. and Mollo, C.M. and Mongelli, M. and Monmarthe, E. and Morganti, M. and Mos, S. and Motz, H. and Moudden, Y. and Mul, G. and Musico, P. and Musumeci, M. and Naumann, C. and Neff, M. and Nicolaou, C. and Orlando, A. and Palioselitis, D. and Papageorgiou, K. and Papaikonomou, A. and Papaleo, R. and Papazoglou, I.A. and Pǎvǎlaş, G.E. and Peek, H.Z. and Perkin, J. and Piattelli, P. and Popa, V. and Pradier, T. and Presani, E. and Priede, I.G. and Psallidas, A. and Rabouille, C. and Racca, C. and Radu, A. and Randazzo, N. and Rapidis, P.A. and Razis, P. and Real, D. and Reed, C. and Reito, S. and Resvanis, L.K. and Riccobene, G. and Richter, R. and Roensch, K. and Rolin, J. and Rose, J. and Roux, J. and Rovelli, A. and Russo, A. and Russo, G.V. and Salesa, F. and Samtleben, D. and Sapienza, P. and Schmelling, J.-W. and Schmid, J. and Schnabel, J. and Schroeder, K. and Schuller, J.-P. and Schussler, F. and Sciliberto, D. and Sedita, M. and Seitz, T. and Shanidze, R. and Simeone, F. and Siotis, I. and Sipala, V. and Sollima, C. and Sparnocchia, S. and Spies, A. and Spurio, M. and Staller, T. and Stavrakakis, S. and Stavropoulos, G. and Steijger, J. and Stolarczyk, T. and Stransky, D. and Taiuti, M. and Taylor, A. and Thompson, L. and Timmer, P. and Tonoiu, D. and Toscano, S. and Touramanis, C. and Trasatti, L. and Traverso, P. and Trovato, A. and Tsirigotis, A. and Tzamarias, S. and Tzamariudaki, E. and Urbano, F. and Vallage, B. and Van Elewyck, V. and Vannoni, G. and Vecchi, M. and Vernin, P. and Viola, S. and Vivolo, D. and Wagner, S. and Werneke, P. and White, R.J. and Wijnker, G. and Wilms, J. and De Wolf, E. and Yepes, H. and Zhukov, V. and Zonca, E. and Zornoza, J.D. and Zúñiga, J.", journal = "ASTROPARTICLE PHYSICS", year = "2013", volume = "42", pages = "7-14", issn = "0927-6505", doi = "10.1016/j.astropartphys.2012.11.010", keywords = "Detectability; Gamma-ray emission; High energy gamma rays; High energy neutrinos; KM3NeT; Large area telescopes; Mediterranean sea; Monte Carlo Simulation; Neutrino spectrum; Neutrino telescopes, Gamma rays; Monte Carlo methods; Neutrons; Telescopes; Tellurium compounds, Particle detectors", 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 50° 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. © 2012 Elsevier B.V. All rights reserved." }