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; J. 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

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 ² 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 ¹ S. Biagi C. Bigongiari B. Bigourdan M. Billault ¹ R. De Boer ^{3, 4, 5, 6} H. Boer Rookhuizen M. Bonori M. Borghini ⁷ M. Bou-Cabo B. Bouhadef G. Bourlis M. Bouwhuis S. Bradbury A. Brown ⁸ F. Bruni ⁹ J. Brunner M. Brunoldi J. Busto G. Cacopardo L. Caillat ¹ D. Calvo Díaz-Aldagalán A. Calzas ¹ M. Canals ¹⁰ A. Capone J. Carr E. Castorina S. Cecchini A. Ceres R. Cereseto Th. Chaleil F. Chateau ¹¹ 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 J. Craig A. Creusot C. Curtil ¹ A. D’amico G. Damy ¹² R. De Asmundis G. De Bonis G. Decock P. Decowski E. Delagnes ¹³ G. De Rosa C. Distefano C. Donzaud D. Dornic Q. Dorosti-Hasankiadeh J. Drogou D. Drouhin F. Druillole ¹³ L. Drury ¹⁴ D. Durand G.A. Durand ¹⁵ T. Eberl U. Emanuele A. Enzenhöfer J.-P. Ernenwein S. Escoffier V. Espinosa G. Etiope ¹⁶ P. Favali D. Felea ¹⁷ M. Ferri ^{18, 19} S. Ferry ²⁰ V. Flaminio F. Folger A. Fotiou U. Fritsch D. Gajanana R. Garaguso G.P. Gasparini ²¹ F. Gasparoni V. Gautard F. Gensolen ¹ K. Geyer G. Giacomelli I. Gialas V. Giordano J. Giraud N. Gizani A. Gleixner C. Gojak ²² J.P. Gómez-González K. Graf D. Grasso A. Grimaldi ²³ R. Groenewegen Z. Guédé G. Guillard F. Guilloux ¹¹ R. Habel G. Hallewell ¹ H. Van Haren ²⁴ 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 ²⁵ 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 ¹ R. Lahmann P. Lamare ¹ G. Larosa D. Lattuada A. Leisos D. Lenis E. Leonora H. Le Provost G. Lim C.D. Llorens ²⁶ J. Lloret ²⁷ H. Löhner D. Lo Presti P. Lotrus ²⁸ F. Louis ²⁸ F. Lucarelli ²⁹ V. Lykousis ³⁰ 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 ¹¹ M. Morganti S. Mos H. Motz Y. Moudden G. Mul P. Musico M. Musumeci Ch. Naumann ³¹ 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 ³² 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 ³³ J. Rose ³⁴ J. Roux A. Rovelli A. Russo G.V. Russo ³⁵ 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 ³⁶ 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 ¹³ 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 IPGP - Institut de Physique du Globe de Paris

3 Department of Epidemiology, Erasmus MC University Medical Center,

4 Department of Radiology, Erasmus MC University Medical Center

5 Department of Medical Informatics, Erasmus MC University Medical Center

6 Biomedical Imaging Group Rotterdam, Erasmus MC University Medical Center

7 CNR-ISMAR

8 Sandia National Laboratories [Livermore]

9 Tecnomare S.p.A.

10 GRC Geociencies Marines

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

12 IFREMER - Centre de Brest

13 DPHN - Département de Physique Nucléaire (ex SPhN)

14 Dublin Institute for Advanced Studies

15 LGGE - Laboratoire de glaciologie et géophysique de l'environnement

16 Istituto Nazionale di Geofisica e Vulcanologia

17 Catedra de Bazele Electrotehnici

18 Sant'Andrea Hospital

19 Surgical and Medical Department of the Clinical Sciences

20 Université de Lyon

21 ISMAR-CNR

22 DT - INSU - Division technique de l'INSU

23 Université de Rouen Normandie - Faculté de Médecine et Pharmacie

24 NIOZ - Royal Netherlands Institute for Sea Research

25 KVI-CART, University of Groningen

26 INLN - Institut Non Linéaire de Nice Sophia-Antipolis

27 Department of environmental sciences

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

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

30 Institute of Oceanography

31 LPNHE - Laboratoire de Physique Nucléaire et de Hautes Énergies

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

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

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

35 Università degli studi di Catania [Catania]

36 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.

Type de document :

Article dans une revue

Astroparticle Physics, Elsevier, 2013, 42, pp.7-14. <10.1016/j.astropartphys.2012.11.010>

Domaine :

Physique [physics] / Physique des Hautes Énergies - Phénoménologie [hep-ph]

Liste complète des métadonnées

http://hal.in2p3.fr/in2p3-00730989
Contributeur : Danielle Cristofol <>
Soumis le : jeudi 13 septembre 2012 - 11:19:01
Dernière modification le : jeudi 24 août 2017 - 17:03:54

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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