Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory

Journal
Date Issued
2015
Author(s)
Aab, A.
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Abreu, P.
•
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Ahn, E. J.
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Al Samarai, I.
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Albuquerque, I. F. M.
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Allekotte, I.
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Allison, P.
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Almela, A.
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Alvarez Castillo, J.
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Alvarez-Muñiz, J.
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Huber, D.
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Huege, T.
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Insolia, A.
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Isar, P. G.
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Jandt, I.
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Jansen, S.
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Jarne, C.
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Johnsen, J. A.
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Josebachuili, M.
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Arsene, N.
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Dhital, N.
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Kääpä, A.
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Kambeitz, O.
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Kampert, K. H.
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Kasper, P.
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Katkov, I.
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Kégl, B.
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Keilhauer, B.
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Keivani, A.
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Kemp, E.
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Kieckhafer, R. M.
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Di Giulio, C.
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Asorey, H.
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Klages, H. O.
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Kleifges, M.
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Kleinfeller, J.
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Krause, R.
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Krohm, N.
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Krömer, O.
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Kuempel, D.
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Kunka, N.
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LaHurd, D.
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Di Matteo, A.
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Latronico, L.
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Assis, P.
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Lauer, R.
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Lauscher, M.
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Lautridou, P.
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Le Coz, S.
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Lebrun, D.
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Lebrun, P.
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Leigui de Oliveira, M. A.
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Letessier-Selvon, A.
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Diaz, J. C.
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Lhenry-Yvon, I.
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Link, K.
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Aublin, J.
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Lopes, L.
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López, R.
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López Casado, A.
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Louedec, K.
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Lu, L.
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Lucero, A.
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Malacari, M.
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Díaz Castro, M. L.
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Maldera, S.
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Mallamaci, M.
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Maller, J.
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Ave, M.
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Mandat, D.
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Mantsch, P.
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Mariazzi, A. G.
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Marin, V.
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Mariș, I. C.
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Marsella, G.
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Diogo, F.
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Martello, D.
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Martin, L.
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Martinez, H.
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Martínez Bravo, O.
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Avenier, M.
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Martraire, D.
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Masías Meza, J. J.
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Mathes, H. J.
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Mathys, S.
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Matthews, J.
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Dobrigkeit, C.
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Matthews, J. A. J.
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Matthiae, G.
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Maurel, D.
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Maurizio, D.
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Mayotte, E.
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Avila, G.
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Mazur, P. O.
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Medina, C.
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Medina-Tanco, G.
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Meissner, R.
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Docters, W.
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Mello, V. B. B.
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Melo, D.
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Menshikov, A.
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•
Meyhandan, R.
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Micheletti, M. I.
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Awal, N.
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Middendorf, L.
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Minaya, I. A.
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Miramonti, L.
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D'Olivo, J. C.
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Mitrica, B.
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Molina-Bueno, L.
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Mollerach, S.
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Montanet, F.
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Morello, C.
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Mostafá, M.
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Moura, C. A.
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Badescu, A. M.
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Muller, M. A.
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Müller, G.
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Dorofeev, A.
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Müller, S.
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Mussa, R.
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Navarra, G.
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Navarro, J. L.
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Navas, S.
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Necesal, P.
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Nellen, L.
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Nelles, A.
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Barber, K. B.
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Neuser, J.
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Alves Batista, R.
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Nguyen, P. H.
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Niculescu-Oglinzanu, M.
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Niechciol, M.
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Niemietz, L.
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Niggemann, T.
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Nitz, D.
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Nosek, D.
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Novotny, V.
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Nožka, L.
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Bäuml, J.
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Dorosti Hasankiadeh, Q.
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Ochilo, L.
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Oikonomou, F.
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Olinto, A.
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Pacheco, N.
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Pakk Selmi-Dei, D.
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Palatka, M.
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Pallotta, J.
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Papenbreer, P.
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Parente, G.
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Parra, A.
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Dova, M. T.
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Baus, C.
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Paul, T.
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Pech, M.
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Pękala, J.
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Pelayo, R.
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Pepe, I. M.
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Perrone, L.
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Petermann, E.
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Peters, C.
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Petrera, S.
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Ebr, J.
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Petrov, Y.
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Beatty, J. J.
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Phuntsok, J.
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Piegaia, R.
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Pierog, T.
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Pieroni, P.
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Pimenta, M.
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Pirronello, V.
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Platino, M.
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Plum, M.
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Engel, R.
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Porcelli, A.
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Porowski, C.
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Becker, K. H.
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Prado, R. R.
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Privitera, P.
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Prouza, M.
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Purrello, V.
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Quel, E. J.
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Querchfeld, S.
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Quinn, S.
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Erdmann, M.
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Rautenberg, J.
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Ravel, O.
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Ravignani, D.
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Bellido, J. A.
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Revenu, B.
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Ridky, J.
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Risse, M.
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Ristori, P.
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Rizi, V.
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Erfani, M.
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Rodrigues de Carvalho, W.
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Rodriguez Fernandez, G.
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Rodriguez Rojo, J.
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Rodríguez-Frías, M. D.
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Berat, C.
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Rogozin, D.
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Rosado, J.
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Roth, M.
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Roulet, E.
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Rovero, A. C.
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Escobar, C. O.
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Saffi, S. J.
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Saftoiu, A.
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Salamida, F.
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Salazar, H.
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Saleh, A.
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Bertaina, M. E.
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Salesa Greus, F.
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Salina, G.
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Sánchez, F.
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Sanchez-Lucas, P.
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Espadanal, J.
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Santos, E.
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Santos, E. M.
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Sarazin, F.
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Sarkar, B.
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Sarmento, R.
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Sato, R.
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Bertou, X.
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Scarso, C.
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Schauer, M.
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Scherini, V.
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Etchegoyen, A.
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Schieler, H.
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Schiffer, P.
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Schmidt, D.
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Scholten, O.
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Schoorlemmer, H.
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Schovánek, P.
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Schröder, F. G.
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Biermann, P. L.
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Schulz, A.
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Schulz, J.
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Falcke, H.
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Schumacher, J.
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Sciutto, S. J.
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Settimo, M.
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Shadkam, A.
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Shellard, R. C.
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Sidelnik, I.
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Sigl, G.
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Billoir, P.
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Sima, O.
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Ambrosio, M.
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Śmiałkowski, A.
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Šmída, R.
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Snow, G. R.
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Sommers, P.
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Sorokin, J.
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Squartini, R.
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Srivastava, Y. N.
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Stanca, D.
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Stanič, S.
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Blaess, S. G.
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Fang, K.
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Stapleton, J.
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Stasielak, J.
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Stephan, M.
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Stutz, A.
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Suarez, F.
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Suomijärvi, T.
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Supanitsky, A. D.
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Sutherland, M. S.
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Swain, J.
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Szadkowski, Z.
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Farrar, G.
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Blanco, A.
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Taborda, O. A.
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Tapia, A.
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Tepe, A.
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Theodoro, V. M.
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Tiffenberg, J.
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Timmermans, C.
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Todero Peixoto, C. J.
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Toma, G.
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Tomankova, L.
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Fauth, A. C.
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Tomé, B.
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Blanco, M.
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Tonachini, A.
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Torralba Elipe, G.
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Torres Machado, D.
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Travnicek, P.
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Ulrich, R.
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Unger, M.
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Urban, M.
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Valdés Galicia, J. F.
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Fazzini, N.
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Valiño, I.
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Valore, L.
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Bleve, C.
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van Aar, G.
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van Bodegom, P.
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van den Berg, A. M.
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van Velzen, S.
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van Vliet, A.
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Varela, E.
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Vargas Cárdenas, B.
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Ferguson, A. P.
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Varner, G.
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Vasquez, R.
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Vázquez, J. R.
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Blümer, H.
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Vázquez, R. A.
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Veberič, D.
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Verzi, V.
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Vicha, J.
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Videla, M.
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Villaseñor, L.
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Fernandes, M.
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Vlcek, B.
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Vorobiov, S.
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Wahlberg, H.
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Wainberg, O.
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Boháčová, M.
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Walz, D.
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Watson, A. A.
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Weber, M.
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Weidenhaupt, K.
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Weindl, A.
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Fick, B.
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Werner, F.
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Widom, A.
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Wiencke, L.
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Wilczyński, H.
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Winchen, T.
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Boncioli, D.
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Wittkowski, D.
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Wundheiler, B.
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Wykes, S.
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Yang, L.
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Figueira, J. M.
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Yapici, T.
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Yushkov, A.
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Zas, E.
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Zavrtanik, D.
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Zavrtanik, M.
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Zepeda, A.
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Bonifazi, C.
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Zhu, Y.
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Zimmermann, B.
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Ziolkowski, M.
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Filevich, A.
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Pierre Auger Collaboration
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Borodai, N.
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Brack, J.
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Brancus, I.
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Bridgeman, A.
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Brogueira, P.
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Brown, W. C.
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Buchholz, P.
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Bueno, A.
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Filipčič, A.
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Buitink, S.
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Buscemi, M.
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Caballero-Mora, K. S.
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Caccianiga, B.
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Caccianiga, L.
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Candusso, M.
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Caramete, L.
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Caruso, R.
•
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Cataldi, G.
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Aminaei, A.
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Cazon, L.
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Cester, R.
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Chavez, A. G.
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Chiavassa, A.
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Chinellato, J. A.
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Chudoba, J.
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Cilmo, M.
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Clay, R. W.
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Cocciolo, G.
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Colalillo, R.
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Fox, B. D.
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Coleman, A.
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Collica, L.
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Coluccia, M. R.
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Conceição, R.
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Contreras, F.
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Cooper, M. J.
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Cordier, A.
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Coutu, S.
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Covault, C. E.
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Cronin, J.
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Fratu, O.
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Dallier, R.
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Daniel, B.
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Dasso, S.
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Daumiller, K.
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Dawson, B. R.
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de Almeida, R. M.
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de Jong, S. J.
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De Mauro, G.
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de Mello Neto, J. R. T.
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De Mitri, I.
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Freire, M. M.
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de Oliveira, J.
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de Souza, V.
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del Peral, L.
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Deligny, O.
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Dembinski, H.
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Fuchs, B.
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Fujii, T.
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García, B.
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Garcia-Pinto, D.
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Gate, F.
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Gemmeke, H.
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Gherghel-Lascu, A.
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Anchordoqui, L.
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Ghia, P. L.
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Giaccari, U.
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Giammarchi, M.
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Giller, M.
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Głas, D.
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Glaser, C.
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Glass, H.
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Golup, G.
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Gómez Berisso, M.
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Gómez Vitale, P. F.
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Andringa, S.
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González, N.
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Gookin, B.
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Gordon, J.
•
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Gorham, P.
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Gouffon, P.
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Griffith, N.
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Grillo, A. F.
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Grubb, T. D.
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Guardincerri, Y.
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Aramo, C.
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Guarino, F.
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Guedes, G. P.
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Hampel, M. R.
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Hansen, P.
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Harari, D.
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Harrison, T. A.
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Hartmann, S.
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Harton, J. L.
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Haungs, A.
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Hebbeker, T.
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Aranda, V. M.
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Heck, D.
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Heimann, P.
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Herve, A. E.
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Hill, G. C.
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Hojvat, C.
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Hollon, N.
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Holt, E.
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Homola, P.
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Hörandel, J. R.
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Horvath, P.
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Arqueros, F.
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Hrabovský, M.
DOI
Description
ACKNOWLEDGMENTS The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Comisión Nacional de Energía Atómica, Fundación Antorchas, Gobierno de la Provincia de Mendoza, Municipalidad de Malargüe, NDM Holdings and Valle Las Leñas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ), São Paulo Research Foundation (FAPESP) Grants No. 2010/07359-6 and No. 1999/05404-3, Ministério de Ciência e Tecnologia (MCT), Brazil; Grants No. MSMT-CR LG13007, No. 7AMB14AR005, and the Czech Science Foundation Grant No. 14-17501S, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Régional Ile-de-France, Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS), Département Sciences de l’Univers (SDU-INSU/CNRS), Institut Lagrange de Paris (ILP) Grant No. LABEX ANR-10-LABX-63, within the Investissements d’Avenir Programme Grant No. ANR-11-IDEX-0004-02, France; Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Württemberg, Helmholtz Alliance for Astroparticle Physics (HAP), Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium für Wissenschaft und Forschung, Nordrhein Westfalen, Ministerium für Wissenschaft, Forschung und Kunst, Baden-Württemberg, Germany; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell’Istruzione, dell’Universitá e della Ricerca (MIUR), Gran Sasso Center for Astroparticle Physics (CFA), CETEMPS Center of Excellence, Ministero degli Affari Esteri (MAE), Italy; Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands; National Centre for Research and Development, Grants No. ERA-NET-ASPERA/01/11 and No. ERA-NET-ASPERA/02/11, National Science Centre, Grants No. 2013/08/M/ST9/00322, No. 2013/08/M/ST9/00728 and No. HARMONIA 5–2013/10/M/ST9/00062, Poland; Portuguese national funds and FEDER funds within Programa Operacional Factores de Competitividade through Fundação para a Ciência e a Tecnologia (COMPETE), Portugal; Romanian Authority for Scientific Research ANCS, CNDI-UEFISCDI partnership projects Grants No. 20/2012 and No. 194/2012, Grants No. 1/ASPERA2/2012 ERA-NET, No. PN-II-RU-PD-2011-3-0145-17 and No. PN-II-RU-PD-2011-3-0062, the Minister of National Education, Programme Space Technology and Advanced Research (STAR), Grant No. 83/2013, Romania; Slovenian Research Agency, Slovenia; Comunidad de Madrid, FEDER funds, Ministerio de Educación y Ciencia, Xunta de Galicia, European Community 7th Framework Program, Grant No. FP7-PEOPLE-2012-IEF-328826, Spain; Science and Technology Facilities Council, United Kingdom; Department of Energy, Contracts No. DE-AC02-07CH11359, No. DE-FR02-04ER41300, No. DE-FG02-99ER41107 and No. DE-SC0011689, National Science Foundation, Grant No. 0450696, The Grainger Foundation, USA; NAFOSTED, Vietnam; Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, European Union 7th Framework Program, Grant No. PIRSES-2009-GA-246806; and UNESCO.
Abstract
Neutrinos in the cosmic ray flux with energies near 1 EeV and above are detectable with the Surface Detector array (SD) of the Pierre Auger Observatory. We report here on searches through Auger data from 1 January 2004 until 20 June 2013. No neutrino candidates were found, yielding a limit to the diffuse flux of ultrahigh energy neutrinos that challenges the Waxman-Bahcall bound predictions. Neutrino identification is attempted using the broad time structure of the signals expected in the SD stations, and is efficiently done for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for "Earth-skimming" neutrino interactions in the case of tau neutrinos. In this paper the searches for downward-going neutrinos in the zenith angle bins 60°-75° and 75°-90° as well as for upward-going neutrinos, are combined to give a single limit. The 90% C.L. single-flavor limit to the diffuse flux of ultrahigh energy neutrinos with an E-2 spectrum in the energy range 1.0 ×1 017 eV - 2.5 ×1 019 eV is Eν2d Nν/d Eν<6.4 ×10-9 GeV cm-2 s-1 sr-1 .
Volume
91
Issue
9
Start page
092008
Uri
Url
Issn Identifier
1550-7998
Ads BibCode
2015PhRvD..91i2008A
Rights
open.access
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