التفاصيل البيبلوغرافية
| العنوان: |
An absence of neutrinos associated with cosmic-ray acceleration in γ-ray bursts |
| المؤلفون: |
Abbasi, R, Abdou, Y, Abu-Zayyad, T, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Altmann, D, Andeen, K, Auffenberg, J, Bai, X, Baker, M, Barwick, SW, Bay, R, Alba, JL, Beattie, K, Beatty, JJ, Bechet, S, Becker, JK, Becker, K-H, Bell, M, Benabderrahmane, ML, Benzvi, S, Berdermann, J, Berghaus, P, Berley, D, Bernardini, E, Bertrand, D, Besson, DZ, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Bose, D, Böser, S, Botner, O, Brayeur, L, Brown, AM, Buitink, S, Caballero-Mora, KS, Carson, M, Casier, M, Chirkin, D, Christy, B, Clevermann, F, Cohen, S, Colnard, C, Cowen, DF, Silva, AH, D’Agostino, MV, Danninger, M, Daughhetee, J, Davis, JC, De Clercq, C, Degner, T, Descamps, F, Desiati, P, De Vries-Uiterweerd, G, Deyoung, T, Díaz-Vélez, JC, Dierckxsens, M, Dreyer, J, Dumm, JP, Dunkman, M, Eisch, J, Ellsworth, RW, Engdegård, O, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Fedynitch, A, Feintzeig, J, Feusels, T, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Franckowiak, A, Franke, R, Gaisser, TK, Gallagher, J, Gerhardt, L, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Goodman, JA, Góra, D, Grant, D, Griesel, T, Groß, A, Grullon, S, Gurtner, M, Ha, C, Ismail, A, Hallgren, A, Halzen, F, Han, K, Hanson, K, Heereman, D, Heinen, D, Helbing, K, Hellauer, R, Hickford, S, Hill, GC, Hoffman, KD, Hoffmann, B, Homeier, A, Hoshina, K, Huelsnitz, W, Hülβ, J-P, Hulth, PO, Hultqvist, K, Hussain, S, Ishihara, A, Jacobi, E, Jacobsen, J, Japaridze, GS, Johansson, H, Kappes, A, Karg, T, Karle, A, Kiryluk, J, Kislat, F, Klein, SR, Köhne, J-H, Kohnen, G, Kolanoski, H, Köpke, L, Kopper, S, Koskinen, DJ, Kowalski, M, Kowarik, T, Krasberg, M, Kroll, G, Kunnen, J, Kurahashi, N, Kuwabara, T, Labare, M, Laihem, K, Landsman, H, Larson, MJ, Lauer, R, Lünemann, J, Madsen, J, Marotta, A, Maruyama, R, Mase, K, Matis, HS, Meagher, K, Merck, M, Mészáros, P, Meures, T, Miarecki, S, Middell, E, Milke, N, Miller, J, Montaruli, T, Morse, R, Movit, SM, Nahnhauer, R, Nam, JW, Naumann, U, Nowicki, SC, Nygren, DR, Odrowski, S, Olivas, A, Olivo, M, O’Murchadha, A, Panknin, S, Paul, L, De Los Heros, C, Piegsa, A, Pieloth, D, Posselt, J, Price, PB, Przybylski, GT, Rawlins, K, Redl, P, Resconi, E, Rhode, W, Ribordy, M, Richman, M, Riedel, B, Rizzo, A, Rodrigues, JP, Rothmaier, F, Rott, C, Ruhe, T, Rutledge, D, Ruzybayev, B, Ryckbosch, D, Sander, H-G, Santander, M, Sarkar, S, Schatto, K, Schmidt, T, Schöneberg, S, Schönwald, A, Schukraft, A, Schulte, L, Schultes, A, Schulz, O, Schunck, M, Seckel, D, Semburg, B, Seo, SH, Sestayo, Y, Seunarine, S, Silvestri, A, Smith, MWE, Spiczak, GM, Spiering, C, Stamatikos, M, Stanev, T, Stezelberger, T, Stokstad, RG, Stößl, A, Strahler, EA, Ström, R, Stüer, M, Sullivan, GW, Taavola, H, Taboada, I, Tamburro, A, Ter-Antonyan, S, Tilav, S, Toale, PA, Toscano, S, Tosi, D, Van Eijndhoven, N, Van Overloop, A, Van Santen, J, Vehring, M, Voge, M, Walck, C, Waldenmaier, T, Wallraff, M, Walter, M, Wasserman, R, Weaver, C, Wendt, C, Westerhoff, S, Whitehorn, N, Wiebe, K, Wiebusch, CH, Williams, DR, Wischnewski, R, Wissing, H, Wolf, M, Wood, TR, Woschnagg, K, Xu, C, Xu, DL, Xu, XW, Yanez, JP, Yodh, G, Yoshida, S, Zarzhitsky, P, Zoll, M |
| بيانات النشر: |
Springer Nature |
| سنة النشر: |
2019 |
| المجموعة: |
Oxford University Research Archive (ORA) |
| الوصف: |
Very energetic astrophysical events are required to accelerate cosmic rays to above 1018 electronvolts. GRBs (γ-ray bursts) have been proposed as possible candidate sources1,2,3. In the GRB ‘fireball’ model, cosmic-ray acceleration should be accompanied by neutrinos produced in the decay of charged pions created in interactions between the high-energy cosmic-ray protons and γ-rays4. Previous searches for such neutrinos found none, but the constraints were weak because the sensitivity was at best approximately equal to the predicted flux5,6,7. Here we report an upper limit on the flux of energetic neutrinos associated with GRBs that is at least a factor of 3.7 below the predictions4,8,9,10. This implies either that GRBs are not the only sources of cosmic rays with energies exceeding 1018 electronvolts or that the efficiency of neutrino production is much lower than has been predicted. |
| نوع الوثيقة: |
article in journal/newspaper |
| اللغة: |
unknown |
| العلاقة: |
https://ora.ox.ac.uk/objects/uuid:41e141f1-c824-4a0a-bc5a-f268ede8c331Test; https://doi.org/10.1038/nature11068Test |
| DOI: |
10.1038/nature11068 |
| الإتاحة: |
https://doi.org/10.1038/nature11068Test
https://ora.ox.ac.uk/objects/uuid:41e141f1-c824-4a0a-bc5a-f268ede8c331Test |
| حقوق: |
info:eu-repo/semantics/openAccess |
| رقم الانضمام: |
edsbas.C566C71F |
| قاعدة البيانات: |
BASE |
