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

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

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dc.contributor.author	Aguilar Sánchez, Juan Antonio
dc.contributor.author	Bigongiari, C.
dc.contributor.author	Calvo Díaz-Aldagalán, David
dc.contributor.author	Emanuele, U.
dc.contributor.author	Gómez González, Juan Pablo
dc.contributor.author	Hernández Rey, Juan José
dc.contributor.author	Mangano, Salvatore
dc.contributor.author	Real Máñez, Diego
dc.contributor.author	Ruiz-Rivas Onsés, Joaquín
dc.contributor.author	Salesa Greus, Francisco
dc.contributor.author	Toscano, S.
dc.contributor.author	Urbano Flores, Fernando
dc.contributor.author	Yepes Ramírez, Harold
dc.contributor.author	Zornoza Gómez, Juan de Dios
dc.contributor.author	Zúñiga Román, Juan
dc.contributor.author	KM3NeT Collaboration
dc.date.accessioned	2013-11-18T13:30:34Z
dc.date.available	2013-11-18T13:30:34Z
dc.date.issued	2013
dc.identifier.citation	Aguilar, J.A. Bigongiari, C. Calvo Diaz-Aldagalan, D. Emanuele, U. Gómez González, Juan Pablo Hernández Rey, Juan José Mangano, S. Real, D. Ruiz Rivas, J. Salesa, F. Toscano, S. Urbano, F. Yepes, H. Zornoza Gómez, Juan de Dios Zúñiga Román, Juan 2013 Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles Astroparticle Physics 42 1 7 14
dc.identifier.uri	http://hdl.handle.net/10550/31119
dc.description.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{\deg} 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-km^3 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 km^3 of instrumented volume. The effect of a possible lower cutoff is also considered.
dc.relation.ispartof	Astroparticle Physics, 2013, vol. 42, num. 1, p. 7-14
dc.subject	Astrofísica
dc.title	Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles
dc.type	journal article	es_ES
dc.date.updated	2013-11-18T13:30:34Z
dc.identifier.doi	10.1016/j.astropartphys.2012.11.010
dc.identifier.idgrec	084303
dc.rights.accessRights	open access	es_ES
dc.identifier.url	10.1016/j.astropartphys.2012.11.010