학술논문

A Search for Neutrino Emission from Fast Radio Bursts with Six Years of IceCube Data
Document Type
Working Paper
Author
IceCube CollaborationAartsen, M. G.Ackermann, M.Adams, J.Aguilar, J. A.Ahlers, M.Ahrens, M.Samarai, I. AlAltmann, D.Andeen, K.Anderson, T.Ansseau, I.Anton, G.Argüelles, C.Auffenberg, J.Axani, S.Bagherpour, H.Bai, X.Barron, J. P.Barwick, S. W.Baum, V.Bay, R.Beatty, J. J.Tjus, J. BeckerBecker, K. -H.BenZvi, S.Berley, D.Bernardini, E.Besson, D. Z.Binder, G.Bindig, D.Blaufuss, E.Blot, S.Bohm, C.Börner, M.Bos, F.Bose, D.Böser, S.Botner, O.Bourbeau, E.Bourbeau, J.Bradascio, F.Braun, J.Brayeur, L.Brenzke, M.Bretz, H. -P.Bron, S.Brostean-Kaiser, J.Burgman, A.Carver, T.Casey, J.Casier, M.Cheung, E.Chirkin, D.Christov, A.Clark, K.Classen, L.Coenders, S.Collin, G. H.Conrad, J. M.Cowen, D. F.Cross, R.Day, M.de André, J. P. A. M.De Clercq, C.DeLaunay, J. J.Dembinski, H.De Ridder, S.Desiati, P.de Vries, K. D.de Wasseige, G.de With, M.DeYoung, T.Díaz-Vélez, J. C.di Lorenzo, V.Dujmovic, H.Dumm, J. P.Dunkman, M.Dvorak, E.Eberhardt, B.Ehrhardt, T.Eichmann, B.Eller, P.Evenson, P. A.Fahey, S.Fazely, A. R.Felde, J.Filimonov, K.Finley, C.Flis, S.Franckowiak, A.Friedman, E.Gaisser, T. K.Gallagher, J.Gerhardt, L.Ghorbani, K.Giang, W.Glauch, T.Glüsenkamp, T.Goldschmidt, A.Gonzalez, J. G.Grant, D.Griffith, Z.Haack, C.Hallgren, A.Halzen, F.Hanson, K.Hebecker, D.Heereman, D.Helbing, K.Hellauer, R.Hickford, S.Hignight, J.Hill, G. C.Hoffman, K. D.Hoffmann, R.Hoinka, T.Hokanson-Fasig, B.Hoshina, K.Huang, F.Huber, M.Hultqvist, K.Hünnefeld, M.In, S.Ishihara, A.Jacobi, E.Japaridze, G. S.Jeong, M.Jero, K.Jones, B. J. P.Kalaczynski, P.Kang, W.Kappes, A.Karg, T.Karle, A.Katz, U.Kauer, M.Keivani, A.Kelley, J. L.Kheirandish, A.Kim, J.Kim, M.Kintscher, T.Kiryluk, J.Kittler, T.Klein, S. R.Kohnen, G.Koirala, R.Kolanoski, H.Köpke, L.Kopper, C.Kopper, S.Koschinsky, J. P.Koskinen, D. J.Kowalski, M.Krings, K.Kroll, M.Krückl, G.Kunnen, J.Kunwar, S.Kurahashi, N.Kuwabara, T.Kyriacou, A.Labare, M.Lanfranchi, J. L.Larson, M. J.Lauber, F.Lesiak-Bzdak, M.Leuermann, M.Liu, Q. R.Mariscal, C. J. LozanoLu, L.Lünemann, J.Luszczak, W.Madsen, J.Maggi, G.Mahn, K. B. M.Mancina, S.Maruyama, R.Mase, K.Maunu, R.McNally, F.Meagher, K.Medici, M.Meier, M.Menne, T.Merino, G.Meures, T.Miarecki, S.Micallef, J.Momenté, G.Montaruli, T.Moore, R. W.Moulai, M.Nahnhauer, R.Nakarmi, P.Naumann, U.Neer, G.Niederhausen, H.Nowicki, S. C.Nygren, D. R.Pollmann, A. ObertackeOlivas, A.O'Murchadha, A.O'Sullivan, E.Palczewski, T.Pandya, H.Pankova, D. V.Peiffer, P.Pepper, J. A.Heros, C. Pérez de losPieloth, D.Pinat, E.Plum, M.Pranav, D.Price, P. B.Przybylski, G. T.Raab, C.Rädel, L.Rameez, M.Rawlins, K.Rea, I. C.Reimann, R.Relethford, B.Relich, M.Resconi, E.Rhode, W.Richman, M.Robertson, S.Rongen, M.Rott, C.Ruhe, T.Ryckbosch, D.Rysewyk, D.Sälzer, T.Herrera, S. E. SanchezSandrock, A.Sandroos, J.Santander, M.Sarkar, S.Satalecka, K.Schlunder, P.Schmidt, T.Schneider, A.Schoenen, S.Schöneberg, S.Schumacher, L.Seckel, D.Seunarine, S.Soedingrekso, J.Soldin, D.Song, M.Spiczak, G. M.Spiering, C.Stachurska, J.Stamatikos, M.Stanev, T.Stasik, A.Stettner, J.Steuer, A.Stezelberger, T.Stokstad, R. G.Stößl, A.Strotjohann, N. L.Stuttard, T.Sullivan, G. W.Sutherland, M.Taboada, I.Tatar, J.Tenholt, F.Ter-Antonyan, S.Terliuk, A.Tešić, G.Tilav, S.Toale, P. A.Tobin, M. N.Toscano, S.Tosi, D.Tselengidou, M.Tung, C. F.Turcati, A.Turley, C. F.Ty, B.Unger, E.Usner, M.Vandenbroucke, J.Van Driessche, W.van Eijndhoven, N.Vanheule, S.van Santen, J.Vehring, M.Vogel, E.Vraeghe, M.Walck, C.Wallace, A.Wallraff, M.Wandler, F. D.Wandkowsky, N.Waza, A.Weaver, C.Weiss, M. J.Wendt, C.Werthebach, J.Westerhoff, S.Whelan, B. J.Wiebe, K.Wiebusch, C. H.Wille, L.Williams, D. R.Wills, L.Wolf, M.Wood, J.Wood, T. R.Woolsey, E.Woschnagg, K.Xu, D. L.Xu, X. W.Xu, Y.Yanez, J. P.Yodh, G.Yoshida, S.Yuan, T.Zoll, M.
Source
Astrophys.J. 857 (2018) 117
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
We present a search for coincidence between IceCube TeV neutrinos and fast radio bursts (FRBs). During the search period from 2010 May 31 to 2016 May 12, a total of 29 FRBs with 13 unique locations have been detected in the whole sky. An unbinned maximum likelihood method was used to search for spatial and temporal coincidence between neutrinos and FRBs in expanding time windows, in both the northern and southern hemispheres. No significant correlation was found in six years of IceCube data. Therefore, we set upper limits on neutrino fluence emitted by FRBs as a function of time window duration. We set the most stringent limit obtained to date on neutrino fluence from FRBs with an $E^{-2}$ energy spectrum assumed, which is 0.0021 GeV cm$^{-2}$ per burst for emission timescales up to \textasciitilde10$^2$ seconds from the northern hemisphere stacking search.
Comment: 15 pages, 9 figures