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Search for prompt neutrino emission from gamma-ray bursts with icecubeopen access

Authors
Aartsen, M.G.Ackermann, M.Adams, J.Aguilar, J.A.Ahlers, M.Ahrens, M.Altmann, D.Anderson, T.Arguelles, C.Arlen, T.C.Auffenberg, J.Bai, X.Barwick, S.W.Baum, V.Bay, R.Beatty, J.J.Tjus, J.B.Becker, K.-H.Benzvi, S.Berghaus, P.Berley, D.Bernardini, E.Bernhard, A.Besson, D.Z.Binder, G.Bindig, D.Bissok, M.Blaufuss, E.Blumenthal, J.Boersma, D.J.Bohm, C.Bos, F.Bose, D.Böser, S.Botner, O.Brayeur, L.Bretz, H.-P.Brown, A.M.Buzinsky, N.Casey, J.Casier, M.Cheung, E.Chirkin, D.Christov, A.Christy, B.Clark, K.Classen, L.Clevermann, F.Coenders, S.Cowen, D.F.Silva, A.H.C.Daughhetee, J.Davis, J.C.Day, M.De, André J.P.A.M.D.De, Clercq C.De, Ridder S.Desiati, P.De, Vries K.D.De, With M.Deyoung, T.Díaz-Vélez, J.C.Dunkman, M.Eagan, R.Eberhardt, B.Ehrhardt, T.Eichmann, B.Eisch, J.Euler, S.Evenson, P.A.Fadiran, O.Fazely, A.R.Fedynitch, A.Feintzeig, J.Felde, J.Filimonov, K.Finley, C.Fischer-Wasels, T.Flis, S.Frantzen, K.Fuchs, T.Gaisser, T.K.Gaior, R.Gallagher, J.Gerhardt, L.Gier, D.Gladstone, L.Glüsenkamp, T.Goldschmidt, A.Golup, G.Gonzalez, J.G.Goodman, J.A.Góra, D.Grant, D.Gretskov, P.Groh, J.C.Groß, A.Ha, C.Haack, C.Ismail, A.H.Hallen, P.Hallgren, A.Halzen, F.Hanson, K.Hebecker, D.Heereman, D.Heinen, D.Helbing, K.Hellauer, R.Hellwig, D.Hickford, S.Hill, G.C.Hoffman, K.D.Hoffmann, R.Homeier, A.Hoshina, K.Huang, F.Huelsnitz, W.Hulth, P.O.Hultqvist, K.Ishihara, A.Jacobi, E.Jacobsen, J.Japaridze, G.S.Jero, K.Jlelati, O.Jurkovic, M.Kaminsky, B.Kappes, A.Karg, T.Karle, A.Kauer, M.Keivani, A.Kelley, J.L.Kheirandish, A.Kiryluk, J.Kläs, J.Klein, S.R.Köhne, J.-H.Kohnen, G.Kolanoski, H.Koob, A.Köpke, L.Kopper, C.Kopper, S.Koskinen, D.J.Kowalski, M.Kriesten, A.Krings, K.Kroll, G.Kroll, M.Kunnen, J.Kurahashi, N.Kuwabara, T.Labare, M.Lanfranchi, J.L.Larsen, D.T.Larson, M.J.Lesiak-Bzdak, M.Leuermann, M.Lünemann, J.Madsen, J.Maggi, G.Maruyama, R.Mase, K.Matis, H.S.Maunu, R.McNally, F.Meagher, K.Medici, M.Meli, A.Meures, T.Miarecki, S.Middell, E.Middlemas, E.Milke, N.Miller, J.Mohrmann, L.Montaruli, T.Morse, R.Nahnhauer, R.Naumann, U.Niederhausen, H.Nowicki, S.C.Nygren, D.R.Obertacke, A.Odrowski, S.Olivas, A.Omairat, A.O'Murchadha, A.Palczewski, T.Paul, L.Penke, Ö.Pepper, J.A.De, Los Heros C.P.Pfendner, C.Pieloth, D.Pinat, E.Posselt, J.Price, P.B.Przybylski, G.T.Pütz, J.Quinnan, M.Rädel, L.Rameez, M.Rawlins, K.Redl, P.Rees, I.Reimann, R.Relich, M.Resconi, E.Rhode, W.Richman, M.Riedel, B.Robertson, S.Rodrigues, J.P.Rongen, M.Rott, C.Ruhe, T.Ruzybayev, B.Ryckbosch, D.Saba, S.M.Sander, H.-G.Sandroos, J.Santander, M.Sarkar, S.Schatto, K.Scheriau, F.Schmidt, T.Schmitz, M.Schoenen, S.Schöneberg, S.Schönwald, A.Schukraft, A.Schulte, L.Schulz, O.Seckel, D.Sestayo, Y.Seunarine, S.Shanidze, R.Smith, M.W.E.Soldin, D.Spiczak, G.M.Spiering, C.Stamatikos, M.Stanev, T.Stanisha, N.A.Stasik, A.Stezelberger, T.Stokstad, R.G.Stößl, A.Strahler, E.A.Ström, R.Strotjohann, N.L.Sullivan, G.W.Taavola, H.Taboada, I.Tamburro, A.Tepe, A.Ter-Antonyan, S.Terliuk, A.Tešić, G.Tilav, S.Toale, P.A.Tobin, M.N.Tosi, D.Tselengidou, M.Unger, E.Usner, M.Vallecorsa, S.Van, Eijndhoven N.Vandenbroucke, J.Van, Santen J.Vehring, M.Voge, M.Vraeghe, M.Walck, C.Wallraff, M.Weaver, Ch.Wellons, M.Wendt, C.Westerhoff, S.Whelan, B.J.Whitehorn, N.Wichary, C.Wiebe, K.Wiebusch, C.H.Williams, D.R.Wissing, H.Wolf, M.Wood, T.R.Woschnagg, K.Xu, D.L.Xu, X.W.Xu, Y.Yanez, J.P.Yodh, G.Yoshida, S.Zarzhitsky, P.Ziemann, J.Zoll, M.
Issue Date
May-2015
Publisher
Institute of Physics Publishing
Keywords
gamma-ray burst: general; neutrinos
Citation
Astrophysical Journal Letters, v.805, no.1
Journal Title
Astrophysical Journal Letters
Volume
805
Number
1
URI
https://scholarworks.bwise.kr/cau/handle/2019.sw.cau/64573
DOI
10.1088/2041-8205/805/1/L5
ISSN
2041-8205
2041-8213
Abstract
We present constraints derived from a search of four years of IceCube data for a prompt neutrino flux from gamma-ray bursts (GRBs). A single low-significance neutrino, compatible with the atmospheric neutrino background, was found in coincidence with one of the 506 observed bursts. Although GRBs have been proposed as candidate sources for ultra-high-energy cosmic rays, our limits on the neutrino flux disfavor much of the parameter space for the latest models. We also find that no more than ∼1% of the recently observed astrophysical neutrino flux consists of prompt emission from GRBs that are potentially observable by existing satellites. © 2015. The American Astronomical Society. All rights reserved..
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자연과학대학 (물리학과)
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