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Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

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Autor(es):
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Aab, A. [1] ; Abreu, P. [2, 3] ; Aglietta, M. [4, 5] ; Albuquerque, I. F. M. [6] ; Albury, J. M. [7] ; Allekotte, I [8, 9] ; Almela, A. [10, 11] ; Alvarez Castillo, J. [12] ; Alvarez-Muniz, J. [13] ; Anastasi, G. A. [14, 15] ; Anchordoqui, L. [16] ; Andrada, B. [10] ; Andringa, S. [2, 3] ; Aramo, C. [17] ; Asorey, H. [8, 9, 18] ; Assis, P. [2, 3] ; Avila, G. [19, 20] ; Badescu, A. M. [21] ; Bakalova, A. [22] ; Balaceanu, A. [23] ; Barbato, F. [17, 24] ; Barreira Luz, R. J. [2, 3] ; Baur, S. [25] ; Becker, K. H. [26] ; Bellido, J. A. [7] ; Berat, C. [27] ; Bertaina, M. E. [5, 28] ; Bertou, X. [8, 9] ; Biermann, P. L. [29] ; Biteau, J. [30] ; Blanco, A. [2, 3] ; Blazek, J. [22] ; Bleve, C. [31, 32] ; Bohacova, M. [22] ; Boncioli, D. [14, 15] ; Bonifazi, C. [33] ; Borodai, N. [34] ; Botti, A. M. [10, 25] ; Brack, J. [35] ; Bretz, T. [36] ; Bridgeman, A. [37] ; Briechle, F. L. [36] ; Buchholz, P. [38] ; Bueno, A. [39, 40] ; Buitink, S. [41] ; Buscemi, M. [42, 43] ; Caballero-Mora, K. S. [44] ; Caccianiga, L. [45] ; Calcagni, L. [46, 47] ; Cancio, A. [10, 11] ; Canfora, F. [1, 48] ; Caracas, I [26] ; Carceller, J. M. [39, 40] ; Caruso, R. [42, 43] ; Castellina, A. [4, 5] ; Catalani, F. [49] ; Cataldi, G. [32] ; Cazon, L. [2, 3] ; Cerda, M. [19] ; Chinellato, J. A. [50] ; Choi, K. [51] ; Chudoba, J. [22] ; Chytka, L. [52] ; Clay, R. W. [7] ; Cobos Cerutti, A. C. [53, 54] ; Colalillo, R. [17, 24] ; Coleman, A. [55] ; Coluccia, M. R. [31, 32] ; Conceicao, R. [2, 3] ; Condorelli, A. [14, 15] ; Consolati, G. [56, 57] ; Contreras, F. [19, 20] ; Convenga, F. [31, 32] ; Cooper, M. J. [7] ; Coutu, S. [58] ; Covault, C. E. [59, 60] ; Daniel, B. [50] ; Dasso, S. [61, 62, 63, 64] ; Daumiller, K. [25] ; Dawson, B. R. [7] ; Day, J. A. [7] ; de Almeida, R. M. [65] ; de Jong, S. J. [1, 48] ; De Mauro, G. [1, 48] ; de Mello Neto, J. R. T. [33, 66] ; De Mitri, I [14, 15] ; de Oliveira, J. [65] ; de Souza, V [67] ; Debatin, J. [37] ; del Rio, M. [19, 20] ; Deligny, O. [30] ; Dhital, N. [34] ; Di Matteo, A. [5] ; Castro, M. L. Diaz [50] ; Dobrigkeit, C. [50] ; D'Olivo, J. C. [12] ; Dorosti, Q. [38] ; dos Anjos, R. C. [68] ; Dova, M. T. [46, 47] ; Dundovic, A. [69] ; Ebr, J. [22] ; Engel, R. [25, 37] ; Erdmann, M. [36] ; Escobar, C. O. [70] ; Etchegoyen, A. [10, 11] ; Falcke, H. [1, 71, 48] ; Farmer, J. [72] ; Farrar, G. [73] ; Fauth, A. C. [50] ; Fazzini, N. [70] ; Feldbusch, F. [74] ; Fenu, F. [5, 28] ; Ferreyro, L. P. [10] ; Figueira, J. M. [10] ; Filipcic, A. [75, 76] ; Freire, M. M. [77, 78] ; Fujii, T. [72, 79, 80] ; Fuster, A. [10, 11] ; Garcia, B. [53, 54] ; Gemmeke, H. [74] ; Gesualdi, F. [10] ; Gherghel-Lascu, A. [23] ; Ghia, P. L. [30] ; Giaccari, U. [81] ; Giammarchi, M. [56] ; Giller, M. [82] ; Las, D. G. [83] ; Glombitza, J. [36] ; Gobbi, F. [19] ; Golup, G. [8, 9] ; Gomez Berisso, M. [8, 9] ; Gomez Vitale, P. F. [19, 20] ; Gongora, J. P. [19] ; Gonzalez, N. [10] ; Goos, I [8, 25, 9] ; Gora, D. [34] ; Gorgi, A. [4, 5] ; Gottowik, M. [26] ; Grubb, T. D. [7] ; Guarino, F. [17, 24] ; Guedes, G. P. [84] ; Guido, E. [5, 28] ; Hahn, S. [25] ; Halliday, R. [59] ; Hampel, M. R. [10] ; Hansen, P. [46, 47] ; Harari, D. [8, 9] ; Harrison, T. A. [7] ; Harvey, V. M. [7] ; Haungs, A. [25] ; Hebbeker, T. [36] ; Heck, D. [25] ; Heimann, P. [38] ; Hill, G. C. [7] ; Hojvat, C. [70] ; Holt, E. M. [10, 37] ; Homola, P. [34] ; Horandel, J. R. [1, 48] ; Horvath, P. [52] ; Hrabovsky, M. [52] ; Huege, T. [25, 41] ; Hulsman, J. [10, 25] ; Insolia, A. [42, 43] ; Isar, P. G. [85] ; Johnsen, J. A. [86] ; Jurysek, J. [22] ; Kaapa, A. [26] ; Kampert, K. H. [26] ; Keilhauer, B. [25] ; Kemmerich, N. [6] ; Kemp, J. [36] ; Klages, H. O. [25] ; Kleifges, M. [74] ; Kleinfeller, J. [19] ; Kuempel, D. [26] ; Mezek, G. Kukec [76] ; Awad, A. Kuotb [37] ; Lago, B. L. [87] ; LaHurd, D. [59] ; Lang, R. G. [67] ; Legumina, R. [82] ; de Oliveira, M. A. Leigui [88] ; Lenok, V [25] ; Letessier-Selvon, A. [89, 90] ; Lhenry-Yvon, I [30] ; Lippmann, O. C. [81] ; Lo Presti, D. [42, 43] ; Lopes, L. [2, 3] ; Lopez, R. [91] ; Lopez Casado, A. [13] ; Lorek, R. [59] ; Luce, Q. [37] ; Lucero, A. [10] ; Malacari, M. [72] ; Mancarella, G. [31, 32] ; Mandat, D. [22] ; Manning, B. C. [7] ; Manshanden, J. [69] ; Mantsch, P. [70] ; Mariazzi, A. G. [46, 47] ; Maris, I. C. [51] ; Marsella, G. [31, 32] ; Martello, D. [31, 32] ; Martinez, H. [67] ; Martinez Bravo, O. [91] ; Mastrodicasa, M. [14, 92] ; Mathes, H. J. [25] ; Mathys, S. [26] ; Matthews, J. [93] ; Matthiae, G. [94, 95] ; Mayotte, E. [26] ; Mazur, P. O. [70] ; Medina-Tanco, G. [12] ; Melo, D. [10] ; Menshikov, A. [74] ; Merenda, K-D [86] ; Michal, S. [52] ; Micheletti, I, M. ; Miramonti, L. [45, 56] ; Mockler, D. [51] ; Mollerach, S. [8, 9] ; Montanet, F. [27] ; Morello, C. [4, 5] ; Morlino, G. [14, 15] ; Mostafa, M. [58] ; Mueller, A. L. [10, 25] ; Muller, M. A. [50, 96] ; Mueller, S. [37] ; Mussa, R. [5] ; Namasaka, W. M. [26] ; Nellen, L. [12] ; Niculescu-Oglinzanu, M. [23] ; Niechciol, M. [38] ; Nitz, D. [97, 98] ; Nosek, D. [99] ; Novotny, V [99] ; Nozka, L. [52] ; Nucita, A. [31, 32] ; Nunez, L. A. [18] ; Olinto, A. [72] ; Palatka, M. [22] ; Pallotta, J. [100, 101] ; Panetta, M. P. [31, 32] ; Papenbreer, P. [26] ; Parente, G. [13] ; Parra, A. [91] ; Pech, M. [22] ; Pedreira, F. [13] ; Pekala, J. [34] ; Pelayo, R. [102] ; Pena-Rodriguez, J. [18] ; Pereira, L. A. S. [50] ; Perlin, M. [10] ; Perrone, L. [31, 32] ; Peters, C. [36] ; Petrera, S. [14, 15] ; Phuntsok, J. [58] ; Pierog, T. [25] ; Pimenta, M. [2, 3] ; Pirronello, V [42, 43] ; Platino, M. [10] ; Poh, J. [72] ; Pont, B. [1] ; Porowski, C. [34] ; Pothast, M. [1, 48] ; Prado, R. R. [67] ; Privitera, P. [72] ; Prouza, M. [22] ; Puyleart, A. [97] ; Querchfeld, S. [26] ; Quinn, S. [59] ; Ramos-Pollan, R. [18] ; Rautenberg, J. [26] ; Ravignani, D. [10] ; Reininghaus, M. [25] ; Ridky, J. [22] ; Riehn, F. [2, 3] ; Risse, M. [38] ; Ristori, P. [100, 101] ; Rizi, V [14, 92] ; de Carvalho, W. Rodrigues [6] ; Rodriguez Rojo, J. [19] ; Roncoroni, M. J. [10] ; Roth, M. [25] ; Roulet, E. [8, 9] ; Rovero, A. C. [61] ; Ruehl, P. [38] ; Sa, S. J. [7] ; Saftoiu, A. [23] ; Salamida, F. [14, 92] ; Salazar, H. [91] ; Salina, G. [95] ; Sanabria Gomez, J. D. [18] ; Sanchez, F. [10] ; Santos, E. M. [6] ; Santos, E. [22] ; Sarazin, F. [86] ; Sarmento, R. [2, 3] ; Sarmiento-Cano, C. [10] ; Sato, R. [19] ; Savina, P. [31, 32] ; Schauer, M. [26] ; Scherini, V [32] ; Schieler, H. [25] ; Schimassek, M. [37] ; Schimp, M. [26] ; Schlueter, F. [25] ; Schmidt, D. [37] ; Scholten, O. [103, 41] ; Schovanek, P. [22] ; Schroeder, F. G. [25, 55] ; Schroeder, S. [26] ; Schumacher, J. [36] ; Sciutto, S. J. [46, 47] ; Scornavacche, M. [10] ; Shellard, R. C. [81] ; Sigl, G. [69] ; Silli, G. [10, 25] ; Sima, O. [23, 60] ; Smida, R. [72] ; Snow, G. R. [104] ; Sommers, P. [58] ; Soriano, J. F. [16] ; Souchard, J. [27] ; Squartini, R. [19] ; Stadelmaier, M. [25] ; Stanca, D. [23] ; Stanic, S. [76] ; Stasielak, J. [34] ; Stassi, P. [27] ; Stolpovskiy, M. [27] ; Streich, A. [37] ; Suarez-Duran, M. [18] ; Sudholz, T. [7] ; Suomijarvi, T. [30] ; Supanitsky, A. D. [10] ; Supik, J. [52] ; Szadkowski, Z. [83] ; Taboada, A. [37] ; Taborda, O. A. [8, 9] ; Tapia, A. [105] ; Timmermans, C. [1, 48] ; Tobiska, P. [22] ; Todero Peixoto, C. J. [49] ; Tome, B. [2, 3] ; Torralba Elipe, G. [13] ; Travaini, A. [19] ; Travnicek, P. [22] ; Trini, M. [76] ; Tueros, M. [46, 47] ; Ulrich, R. [25] ; Unger, M. [25] ; Urban, M. [36] ; Valdes Galicia, J. F. [12] ; Valino, I [14, 15] ; Valore, L. [17, 24] ; van Bodegom, P. [7] ; van den Berg, A. M. [103] ; van Vliet, A. [1] ; Varela, E. [91] ; Vargas Cardenas, B. [12] ; Vasquez-Ramirez, A. [18] ; Veberic, D. [25] ; Ventura, C. [66] ; Vergara Quispe, I. D. [46, 47] ; Verzi, V. [95] ; Vicha, J. [22] ; Villasenor, L. [91] ; Vink, J. [106] ; Vorobiov, S. [76] ; Wahlberg, H. [46, 47] ; Watson, A. A. [107] ; Weber, M. [74] ; Weindl, A. [25] ; Wiedenski, M. [83] ; Wiencke, L. [86] ; Wilczynski, H. [34] ; Winchen, T. [41] ; Wirtz, M. [36] ; Wittkowski, D. [26] ; Wundheiler, B. [10] ; Yang, L. [76] ; Yushkov, A. [22] ; Zas, E. [13] ; Zavrtanik, D. [75, 76] ; Zavrtanik, M. [75, 76] ; Zehrer, L. [76] ; Zepeda, A. [108] ; Zimmermann, B. [25] ; Ziolkowski, M. [38] ; Zuccarello, F. [42, 43] ; Collaboration, Pierre Auger
Número total de Autores: 392
Afiliação do(s) autor(es):
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[1] Radboud Univ Nijmegen, IMAPP, Nijmegen - Netherlands
[2] Univ Lisbon, IST, Lisbon - Portugal
[3] Univ Lisbon, Lab Instrumentacao & Fis Expt Particular LIP, Lisbon - Portugal
[4] Osservatorio Astrofis Torino INAF, Turin - Italy
[5] INFN, Sez Torino, Turin - Italy
[6] Univ Sao Paulo, Inst Fis, Sao Paulo, SP - Brazil
[7] Univ Adelaide, Adelaide, SA - Australia
[8] CNEA UNCuyo CONICET, Inst Balseiro, San Carlos De Bariloche, Rio Negro - Argentina
[9] Ctr Atom Bariloche, San Carlos De Bariloche, Rio Negro - Argentina
[10] UNSAM, CONICET, CNEA, Inst Tecnol Detecc & Astroparticulas, Buenos Aires, DF - Argentina
[11] Univ Tecnol Nacl, Fac Reg Buenos Aires, Buenos Aires, DF - Argentina
[12] Univ Nacl Autonoma Mexico, Mexico City, DF - Mexico
[13] Univ Santiago de Compostela, IGFAE, Santiago De Compostela - Spain
[14] INFN, Lab Nazl Gran Sasso, Laquila - Italy
[15] Gran Sasso Sci Inst, Laquila - Italy
[16] CUNY, Lehman Coll, Dept Phys & Astron, Bronx, NY - USA
[17] INFN, Sez Napoli, Naples - Italy
[18] Univ Ind Santander, Bucaramanga - Colombia
[19] Observ Pierre Auger, Malargue - Argentina
[20] Comis Nacl Energia Atom, Malargue - Argentina
[21] Univ Politehn Bucuresti, Bucharest - Romania
[22] Czech Acad Sci, Inst Phys, Prague - Czech Republic
[23] Horia Hulubei Natl Inst Phys & Nucl Engn, Bucharest - Romania
[24] Univ Napoli Federico II, Dipartimento Fis Ettore Pancini, Naples - Italy
[25] Karlsruhe Inst Technol, Inst Kernphys, Karlsruhe - Germany
[26] Berg Univ Wuppertal, Dept Phys, Wuppertal - Germany
[27] Univ Grenoble Alpes, LPSC IN2P3, Grenoble Inst Engn, CNRS, F-38000 Grenoble - France
[28] Univ Torino, Dipartimento Fis, Turin - Italy
[29] Max Planck Inst Radioastron, Bonn - Germany
[30] Univ Paris Sud, Univ Paris Saclay, IPNO, CNRS IN2P3, Orsay - France
[31] Univ Salento, Dipartimento Matemat & Fis E De Giorgi, Lecce - Italy
[32] INFN, Sez Lecce, Lecce - Italy
[33] Univ Fed Rio de Janeiro, Inst Fis, Rio De Janeiro, RJ - Brazil
[34] Inst Nucl Phys PAN, Krakow - Poland
[35] Colorado State Univ, Ft Collins, CO 80523 - USA
[36] Rhein Westfal TH Aachen, Phys Inst A 3, Aachen - Germany
[37] Karlsruhe Inst Technol, Inst Expt Particle Phys ETP, Karlsruhe - Germany
[38] Univ Siegen, Fachbereich Phys Expt Teilchenphys 7, Siegen - Germany
[39] Univ Granada, Granada - Spain
[40] CAFPE, Granada - Spain
[41] Vrije Univ Brussels, Brussels - Belgium
[42] Univ Catania, Dipartimento Fis & Astron, Catania - Italy
[43] INFN, Sez Catania, Catania - Italy
[44] Univ Autonoma Chiapas, Tuxtla Gutierrez, Chiapas - Mexico
[45] Univ Milan, Dipartimento Fis, Milan - Italy
[46] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires - Argentina
[47] Univ Nacl La Plata, IFLP, La Plata, Buenos Aires - Argentina
[48] Natl Inst Kernfys Hoge Energie Fys NIKHEF, Sci Pk, Amsterdam - Netherlands
[49] Univ Sao Paulo, Escola Engn Lorena, Lorena, SP - Brazil
[50] Univ Estadual Campinas, IFGW, Campinas, SP - Brazil
[51] ULB, Brussels - Belgium
[52] Palacky Univ, RCPTM, Olomouc - Czech Republic
[53] UNSAM, CONICET, CNEA, Inst Tecnol Detecc & Astroparticulas, Mendoza - Argentina
[54] Univ Tecnol Nacl, Fac Reg Mendoza, CONICET, CNEA, Mendoza - Argentina
[55] Univ Delaware, Dept Phys & Astron, Bartol Res Inst, Newark, DE 19716 - USA
[56] INFN, Sez Milano, Milan - Italy
[57] Politecn Milan, Dipartimento Sci & Tecnol Aerosp, Milan - Italy
[58] Penn State Univ, University Pk, PA 16802 - USA
[59] Case Western Reserve Univ, Cleveland, OH 44106 - USA
[60] Radboud Univ Nijmegen, Nijmegen - Netherlands
[61] CONICET UBA, IAFE, Buenos Aires, DF - Argentina
[62] Consejo Nacl Invest Cient & Tecn, Buenos Aires, DF - Argentina
[63] Univ Buenos Aires, FCEyN, Dept Fis, Buenos Aires, DF - Argentina
[64] Univ Buenos Aires, FCEyN, Dept Ciencias Atmosfera & Oceanos, Buenos Aires, DF - Argentina
[65] Univ Fed Fluminense, EEIMVR, Volta Redonda, RJ - Brazil
[66] Univ Fed Rio de Janeiro, Observ Valongo, Rio de Janeiro, RJ - Brazil
[67] Univ Sao Paulo, Inst Fis Sao Carlos, Sao Carlos, SP - Brazil
[68] Univ Fed Parana, Setor Palotina, Palotina - Brazil
[69] Univ Hamburg, Inst Theoret Phys 2, Hamburg - Germany
[70] Fermilab Natl Accelerator Lab, Batavia, IL 60510 - USA
[71] Stichting Astron Onderzoek Nederland ASTRON, Dwingeloo - Netherlands
[72] Univ Chicago, Enrico Fermi Inst, 5640 S Ellis Ave, Chicago, IL 60637 - USA
[73] NYU, New York, NY - USA
[74] Karlsruhe Inst Technol, Inst Prozessdatenverarbeitung & Elekt, Karlsruhe - Germany
[75] J Stefan Inst, Expt Particle Phys Dept, Ljubljana - Slovenia
[76] Univ Nova Gorica, CAC, Nova Gorica - Slovenia
[77] I, UNR, Fac Ciencias Bioquim & Farmaceut, Rosario, Santa Fe - Argentina
[78] I, UNR, CONICET, Inst Fis Rosario IFIR, Rosario, Santa Fe - Argentina
[79] Kyoto Univ, Hakubi Ctr Adv Res, Kyoto - Japan
[80] Kyoto Univ, Grad Sch Sci, Kyoto - Japan
[81] Ctr Brasileiro Pesquisas Fis, Rio De Janeiro, RJ - Brazil
[82] Univ Lodz, Fac Astrophys, Lodz - Poland
[83] Univ Lodz, Fac High Energy Astrophys, Lodz - Poland
[84] Univ Estadual Feira de Santana, Feira De Santana, BA - Brazil
[85] Inst Space Sci, Bucharest - Romania
[86] Colorado Sch Mines, Golden, CO 80401 - USA
[87] Ctr Fed Educ Tecnol Celso Suckow da Fonseca, Nova Friburgo - Brazil
[88] Univ Fed ABC, Santo Andre, SP - Brazil
[89] Univ Paris 06, LPNHE, Paris - France
[90] Univ Paris 07, LPNHE, CNRS, IN2P3, Paris - France
[91] Benemerita Univ Autonoma Puebla, Puebla - Mexico
[92] Univ Aquila, Dipartimento Sci Fis & Chim, Laquila - Italy
[93] Louisiana State Univ, Baton Rouge, LA 70803 - USA
[94] Univ Roma Tor Vergata, Dipartimento Fis, Rome - Italy
[95] INFN, Sez Roma Tor Vergata, Rome - Italy
[96] Univ Fed Alfenas, Pocos De Caldas - Brazil
[97] Michigan Technol Univ, Houghton, MI 49931 - USA
[98] Karlsruhe Inst Technol, Karlsruhe - Germany
[99] Charles Univ Prague, Fac Math & Phys, Inst Particle & Nucl Phys, Prague - Czech Republic
[100] Consejo Nacl Invest Cient & Tecn, Villa Martelli - Argentina
[101] CITEDEF, Ctr Invest Laseres & Aplicac, Villa Martelli - Argentina
[102] IPN, UPIITA, Mexico City, DF - Mexico
[103] Univ Groningen, KVI Ctr Adv Radiat Technol, Groningen - Netherlands
[104] Univ Nebraska, Lincoln, NE - USA
[105] Univ Medellin, Medellin - Colombia
[106] Univ Amsterdam, Fac Sci, Amsterdam - Netherlands
[107] Univ Leeds, Sch Phys & Astron, Leeds, W Yorkshire - England
[108] CINVESTAV, Ctr Invest & Estudios Avanzados, Mexico City, DF - Mexico
Número total de Afiliações: 108
Tipo de documento: Artigo Científico
Fonte: Journal of Cosmology and Astroparticle Physics; n. 10 OCT 2019.
Citações Web of Science: 0
Resumo

Neutrinos with energies above 10(17) eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for Earth-skimming tau neutrinos with nearly tangential trajectories relative to the Earth. No neutrino candidates were found in similar to 14.7 years of data taken up to 31 August 2018. This leads to restrictive upper bounds on their flux. The 90% C.L. single-flavor limit to the diffuse flux of ultra-high-energy neutrinos with an E-nu(-2) spectrum in the energy range 1.0 x 10(17) eV-2.5 x 10(19) eV is E(2)dN(nu)/dE(nu) < 4.4 x 10(-9) GeV cm(-2) s(-1) sr(-1), placing strong constraints on several models of neutrino production at EeV energies and on the properties of the sources of ultra-high-energy cosmic rays. (AU)

Processo FAPESP: 10/07359-6 - Estudo dos raios cósmicos de mais altas energias com o Observatório Pierre Auger
Beneficiário:Carola Dobrigkeit Chinellato
Linha de fomento: Auxílio à Pesquisa - Temático
Processo FAPESP: 99/05404-3 - Observatório Pierre Auger
Beneficiário:Carlos Ourivio Escobar
Linha de fomento: Auxílio à Pesquisa - Temático