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

S. Adrián-Martínez; M. Ageron; J.A. Aguilar; F. Aharonian; S. Aiello; A. Albert; M. Alexandri; F. Ameli; E.G. Anassontzis; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. Assis Jesus; J.-J. Aubert; R. Bakker; A.E. Ball; G. Barbarino; E. Barbarito; F. Barbato; B. Baret; M. de Bel; A. Belias; N. Bellou; E. Berbee; A. Berkien; A. Bersani; V. Bertin; S. Beurthey; S. Biagi; C. Bigongiari; B. Bigourdan; M. Billault; R. de Boer; H. Boer Rookhuizen; M. Bonori; M. Borghini; M. Bou-Cabo; B. Bouhadef; G. Bourlis; M. Bouwhuis; S. Bradbury; A. Brown; F. Bruni; J. Brunner; M. Brunoldi; J. Busto; G. Cacopardo; L. Caillat; D. Calvo Díaz-Aldagalán; A. Calzas; M. Canals; A. Capone; J. Carr; E. Castorina; S. Cecchini; A. Ceres; R. Cereseto; Th. Chaleil; F. Chateau; T. Chiarusi; D. Choqueuse; P.E. Christopoulou; G. Chronis; O. Ciaffoni; M. Circella; R. Cocimano; F. Cohen; F. Colijn; R. Coniglione; M. Cordelli; A. Cosquer; M. Costa; P. Coyle; J. Craig; A. Creusot; C. Curtil; A. D’amico; G. Damy; R. de Asmundis; G. de Bonis; G. Decock; P. Decowski; E. Delagnes; G. de Rosa; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti-Hasankiadeh; J. Drogou; D. Drouhin; F. Druillole; L. Drury; D. Durand; G.A. Durand; T. Eberl; U. Emanuele; A. Enzenhöfer; J.-P. Ernenwein; S. Escoffier; V. Espinosa; G. Etiope; P. Favali; D. Felea; M. Ferri; S. Ferry; V. Flaminio; F. Folger; A. Fotiou; U. Fritsch; D. Gajanana; R. Garaguso; G.P. Gasparini; F. Gasparoni; V. Gautard; F. Gensolen; K. Geyer; G. Giacomelli; I. Gialas; V. Giordano; J. Giraud; N. Gizani; A. Gleixner; C. Gojak; J.P. Gómez-González; K. Graf; D. Grasso; A. Grimaldi; R. Groenewegen; Z. Guédé; G. Guillard; F. Guilloux; R. Habel; G. Hallewell; H. van Haren; J. van Heerwaarden; A. Heijboer; E. Heine; J.J. Hernández-Rey; B. Herold; T. Hillebrand; M. van de Hoek; J. Hogenbirk; J. Hößl; C.C. Hsu; M. Imbesi; A. Jamieson; P. Jansweijer; M. de Jong; F. Jouvenot; M. Kadler; N. Kalantar-Nayestanaki; O. Kalekin; A. Kappes; M. Karolak; U.F. Katz; O. Kavatsyuk; P. Keller; Y. Kiskiras; R. Klein; H. Kok; H. Kontoyiannis; P. Kooijman; J. Koopstra; C. Kopper; A. Korporaal; P. Koske; A. Kouchner; S. Koutsoukos; I. Kreykenbohm; V. Kulikovskiy; M. Laan; C. La Fratta; P. Lagier; R. Lahmann; P. Lamare; G. Larosa; D. Lattuada; A. Leisos; D. Lenis; E. Leonora; H. Le Provost; G. Lim; C.D. Llorens; J. Lloret; H. Löhner; D. Lo Presti; P. Lotrus; F. Louis; F. Lucarelli; V. Lykousis; D. Malyshev; S. Mangano; E.C. Marcoulaki; A. Margiotta; G. Marinaro; A. Marinelli; O. Mariş; E. Markopoulos; C. Markou; J.A. Martínez-Mora; A. Martini; J. Marvaldi; R. Masullo; G. Maurin; P. Migliozzi; E. Migneco; S. Minutoli; A. Miraglia; C.M. Mollo; M. Mongelli; E. Monmarthe; M. Morganti; S. Mos; H. Motz; Y. Moudden; G. Mul; P. Musico; M. Musumeci; Ch. Naumann; M. Neff; C. Nicolaou; A. Orlando; D. Palioselitis; K. Papageorgiou; A. Papaikonomou; R. Papaleo; I.A. Papazoglou; G.E. Păvălaş; H.Z. Peek; J. Perkin; P. Piattelli; V. Popa; T. Pradier; E. Presani; I.G. Priede; A. Psallidas; C. Rabouille; C. Racca; A. Radu; N. Randazzo; P.A. Rapidis; P. Razis; D. Real; C. Reed; S. Reito; L.K. Resvanis; G. Riccobene; R. Richter; K. Roensch; J. Rolin; Jérôme Rose; J. Roux; A. Rovelli; A. Russo; G.V. Russo; F. Salesa; D. Samtleben; P. Sapienza; J.-W. Schmelling; J. Schmid; J. Schnabel; K. Schroeder; J.-P. Schuller; F. Schussler; D. Sciliberto; M. Sedita; T. Seitz; R. Shanidze; F. Simeone; I. Siotis; V. Sipala; C. Sollima; S. Sparnocchia; A. Spies; M. Spurio; T. Staller; S. Stavrakakis; G. Stavropoulos; J. Steijger; Th. Stolarczyk; D. Stransky; M. Taiuti; A. Taylor; L. Thompson; P. Timmer; D. Tonoiu; S. Toscano; C. Touramanis; L. Trasatti; P. Traverso; A. Trovato; A. Tsirigotis; S. Tzamarias; E. Tzamariudaki; F. Urbano; B. Vallage; V. van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; S. Viola; D. Vivolo; S. Wagner; P. Werneke; R.J. White; G. Wijnker; J. Wilms; E. de Wolf; H. Yepes; V. Zhukov; E. Zonca; J.D. Zornoza; J. Zúñiga

doi:10.1016/j.astropartphys.2012.11.010

Journal articles

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

S. Adrián-Martínez M. Ageron ¹ J.A. Aguilar F. Aharonian S. Aiello A. Albert M. Alexandri F. Ameli E.G. Anassontzis M. Anghinolfi G. Anton S. Anvar M. Ardid A. Assis Jesus J.-J. Aubert ¹ R. Bakker A.E. Ball G. Barbarino E. Barbarito F. Barbato ² B. Baret M. de Bel A. Belias N. Bellou E. Berbee A. Berkien A. Bersani V. Bertin ¹ S. Beurthey ¹ S. Biagi C. Bigongiari B. Bigourdan M. Billault ¹ R. de Boer ³ H. Boer Rookhuizen M. Bonori M. Borghini ⁴ M. Bou-Cabo B. Bouhadef G. Bourlis M. Bouwhuis S. Bradbury A. Brown ¹ F. Bruni ⁵ J. Brunner ¹ M. Brunoldi J. Busto ¹ G. Cacopardo L. Caillat ¹ D. Calvo Díaz-Aldagalán A. Calzas ¹ M. Canals ⁶ A. Capone J. Carr ¹ E. Castorina S. Cecchini A. Ceres R. Cereseto Th. Chaleil F. Chateau ⁷ T. Chiarusi D. Choqueuse P.E. Christopoulou G. Chronis O. Ciaffoni M. Circella R. Cocimano F. Cohen F. Colijn R. Coniglione M. Cordelli A. Cosquer ¹ M. Costa P. Coyle ¹ J. Craig ² A. Creusot C. Curtil ¹ A. D’amico G. Damy ⁸ R. de Asmundis G. de Bonis G. Decock P. Decowski E. Delagnes ⁹ G. de Rosa C. Distefano ² C. Donzaud D. Dornic ¹ Q. Dorosti-Hasankiadeh J. Drogou D. Drouhin F. Druillole ⁹ L. Drury ¹⁰ D. Durand G.A. Durand T. Eberl U. Emanuele A. Enzenhöfer J.-P. Ernenwein ¹ S. Escoffier ¹ V. Espinosa G. Etiope ¹¹ P. Favali D. Felea ¹² M. Ferri ^{13, 14} S. Ferry ¹⁵ V. Flaminio F. Folger A. Fotiou U. Fritsch D. Gajanana R. Garaguso G.P. Gasparini ¹⁶ F. Gasparoni V. Gautard F. Gensolen ¹ K. Geyer G. Giacomelli I. Gialas V. Giordano J. Giraud N. Gizani A. Gleixner C. Gojak ¹ J.P. Gómez-González K. Graf D. Grasso A. Grimaldi ¹⁷ R. Groenewegen Z. Guédé G. Guillard F. Guilloux ⁷ R. Habel G. Hallewell ¹ H. van Haren ¹⁸ J. van Heerwaarden A. Heijboer E. Heine J.J. Hernández-Rey B. Herold T. Hillebrand M. van de Hoek J. Hogenbirk J. Hößl C.C. Hsu M. Imbesi A. Jamieson P. Jansweijer M. de Jong F. Jouvenot M. Kadler N. Kalantar-Nayestanaki ¹⁹ O. Kalekin A. Kappes M. Karolak U.F. Katz O. Kavatsyuk P. Keller ¹ Y. Kiskiras R. Klein H. Kok H. Kontoyiannis P. Kooijman J. Koopstra C. Kopper A. Korporaal P. Koske ² A. Kouchner S. Koutsoukos I. Kreykenbohm V. Kulikovskiy M. Laan C. La Fratta P. Lagier ¹ R. Lahmann P. Lamare ¹ G. Larosa D. Lattuada A. Leisos D. Lenis E. Leonora H. Le Provost G. Lim C.D. Llorens ²⁰ J. Lloret ²¹ H. Löhner D. Lo Presti P. Lotrus ²² F. Louis ²² F. Lucarelli ²³ V. Lykousis ²⁴ D. Malyshev S. Mangano E.C. Marcoulaki A. Margiotta G. Marinaro A. Marinelli O. Mariş E. Markopoulos C. Markou J.A. Martínez-Mora A. Martini J. Marvaldi R. Masullo G. Maurin P. Migliozzi E. Migneco S. Minutoli A. Miraglia C.M. Mollo M. Mongelli E. Monmarthe ⁷ M. Morganti S. Mos H. Motz Y. Moudden G. Mul P. Musico M. Musumeci Ch. Naumann M. Neff C. Nicolaou A. Orlando D. Palioselitis K. Papageorgiou A. Papaikonomou R. Papaleo I.A. Papazoglou G.E. Păvălaş H.Z. Peek J. Perkin P. Piattelli V. Popa T. Pradier E. Presani I.G. Priede A. Psallidas C. Rabouille ^{25, 26} C. Racca A. Radu N. Randazzo P.A. Rapidis P. Razis D. Real C. Reed S. Reito L.K. Resvanis G. Riccobene R. Richter K. Roensch J. Rolin ²⁷ Jérôme Rose ²⁸ J. Roux ¹ A. Rovelli A. Russo G.V. Russo ²⁹ F. Salesa D. Samtleben P. Sapienza J.-W. Schmelling J. Schmid J. Schnabel K. Schroeder J.-P. Schuller F. Schussler D. Sciliberto M. Sedita T. Seitz R. Shanidze F. Simeone I. Siotis V. Sipala C. Sollima S. Sparnocchia A. Spies M. Spurio T. Staller S. Stavrakakis ³⁰ G. Stavropoulos J. Steijger Th. Stolarczyk D. Stransky M. Taiuti A. Taylor L. Thompson P. Timmer D. Tonoiu S. Toscano C. Touramanis L. Trasatti P. Traverso A. Trovato A. Tsirigotis S. Tzamarias E. Tzamariudaki F. Urbano B. Vallage ² V. van Elewyck G. Vannoni M. Vecchi ¹ P. Vernin ⁹ S. Viola D. Vivolo S. Wagner P. Werneke R.J. White G. Wijnker J. Wilms E. de Wolf H. Yepes V. Zhukov E. Zonca J.D. Zornoza J. Zúñiga

1 CPPM - Centre de Physique des Particules de Marseille

2 APC (UMR_7164) - AstroParticule et Cosmologie

3 Erasmus MC - Erasmus University Medical Center [Rotterdam]

4 ISMAR - Istituto di Science Marine

5 Tecnomare S.p.A.

6 GRC Geociencies Marines

7 IRFU - Institut de Recherches sur les lois Fondamentales de l'Univers

8 IFREMER - Institut Français de Recherche pour l'Exploitation de la Mer - Brest

9 DPHN - Département de Physique Nucléaire (ex SPhN)

10 DIAS - Dublin Institute for Advanced Studies

11 Istituto Nazionale di Geofisica e Vulcanologia

12 Catedra de Bazele Electrotehnici

13 Sant'Andrea Hospital

14 Surgical and Medical Department of the Clinical Sciences

15 Université de Lyon

16 ISMAR - Istituto di Scienze Marine [Genova]

17 UNIROUEN UFR Santé - UNIROUEN - UFR Santé

18 NIOZ - Royal Netherlands Institute for Sea Research

19 KVI-CART, University of Groningen

20 INPHYNI - Institut de Physique de Nice

21 Department of environmental sciences

22 DPP - Département de Physique des Particules (ex SPP)

23 Universita degli studi di Napoli "Parthenope" [Napoli]

24 Institute of Oceanography

25 LSCE - Laboratoire des Sciences du Climat et de l'Environnement [Gif-sur-Yvette]

26 OCEANIS - Océan et Interfaces

LSCE - Laboratoire des Sciences du Climat et de l'Environnement [Gif-sur-Yvette] : DRF/LSCE

27 IFREMER - Institut Français de Recherche pour l'Exploitation de la Mer

28 CEREGE - Centre européen de recherche et d'enseignement des géosciences de l'environnement

29 Università degli studi di Catania [Catania]

30 HCMR - Hellenic Centre for Marine Research

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.

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Journal articles

Domain :

Physics [physics] / High Energy Physics - Phenomenology [hep-ph]

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