Search for Sources of High-Energy Neutrons with four Years of Data from the IceTop Detector

M. G. Aartsen,G. C. Hill,K. Meagher,Subir Sarkar,F. Huang,C. Argüelles,M. van Rossem,P. Berghaus,J. P. A. M. de André,S. C. Nowicki,R. Cross,F. Lauber, P. Schlunder, M. Lesiak-Bzdak,S. Hickford,A. Sandrock, L. Gerhardt,S. Westerhoff,J. M. Conrad,N. Wandkowsky,P. A. Toale, M. N. Tobin,M. Day,A. Bernhard,M. Meier,S. Kunwar,L. Köpke, J. Hignight,Stijn Blot,C. Krüger,T. R. Wood, M. Mandelartz,J. A. Aguilar,T. Palczewski,D. V. Pankova,Jürgen Braun,L. Wills, J. Tatar,S. Seunarine,R. Nahnhauer, B. Relethford,R. Hoffmann,J. Becker Tjus,M. Labare, F. Tenholt,L. Wille, J. Auffenberg, F. Halzen,H. Kolanoski,P. Desiati, P. Eller,K. Rawlins,Ö. Penek,D. Berley,J. Feintzeig,R. Koirala, A. Meli,K.B.M. Mahn,M. Sutherland,A. Stasik,M. Börner,K. Andeen,A. Haj Ismail,Eitan Friedman,G. Tes,S. BenZvi, T. Fuchs,H.-P. Bretz,M. Song,B.J.P. Jones, G. Neer,M. Rameez,M. J. Weiss,C. De Clercq, F. McNally,T. Anderson,J. Gallagher,S. Schoenen,D. Ryckbosch,D. Seckel,D. L. Xu,E. del Pino Rosendo,C. Haack,J. Kemp,S. Coenders, S. Mancina,E. Hansen,G. de Wasseige,M. Ahlers,D. Pieloth,R. G. Stokstad,J. Kunnen,M. Voge, D. Heereman,T. Kuwabara,E. Jacobi,M. Bissok,T. Montaruli,U. Naumann,O. Botner,J. G. Gonzalez, E. Woolsey,H. Dembinski,A. Burgman,T. Stezelberger,R. Maruyama,D. Rysewyk,D. J. Koskinen,M. Casier, R. Maunu,L. Gladstone,T. Carver,L. Classen,D. Tosi,K. Woschnagg,P. B. Price,J. A. Pepper, Z. Griffith, K. Hanson,M. Glagla,G. T. Przybylski,K. Clark,C. Finley,X. W. Xu,K. Satalecka, D. Hebecker,D. Grant,T. Kintscher,D. Chirkin, M. Medici,B. Riedel, A. O'Murchadha,K. Wiebe,J. J. Beatty,S. Robertson, J. Sandroos,W. Giang,Michael Rongen,A. Franckowiak,M. Vraeghe,M. Huber,T. Menne,K. Ghorbani,G. Golup,A. Christov,C. H. Wiebusch,H. Niederhausen,H. Pandya,M. Quinnan,E. Pinat,G. W. Sullivan,E. Resconi,S. Toscano,J. Felde,B. Hansmann,T. Karg, G. Krückl,B. Eichmann, J. Kiryluk,K. Mase, B. Eberhardt,G. M. Spiczak,C. Kopper,S. Kopper,L. Schumacher,Christian Bohm,T. Meures,M. Tselengidou, R. Bay,P. A. Evenson,U. Katz,M. Dunkman,Spencer R. Klein, A. Steuer,J. Adams, A. Turcati,T. Schmidt,K. Filimonov,A. Karle,M. Stahlberg,C. Pérez de los Heros,A. Goldschmidt,K. Hoshina,M. Moulai,M. Kowalski, S. Fahey,N. van Eijndhoven,M. Ackermann,G. Anton,A. Kheirandish,S. Axani, A. Hallgren, A. Stossl,D. F. Cowen,S. Schöneberg, M. Zoll,V. Baum,M. Jeong,E. Blaufuss, M. Ahrens,F. Bos, T. Hansmann, G. Yodh,C. Rott,D. Soldin,R. Ström, M. Usner, L. Sabbatini,A. R. Fazely,R. Hellauer,A. Wallace,Ch. Weaver,E. Bernardini,M. J. Larson,J. van Santen,D. Altmann,S. E. Sanchez Herrera,G. Merino,Mj Kim,M. Vehring,S. W. Barwick, G. Binder,T. Ehrhardt,D. Bose,T. DeYoung,G.H. Collin, I. Ansseau,X. Bai,M. Wallraff,C. Walck,G. Kohnen,J. Vandenbroucke, M. Leuermann,D. Bindig,J. C. Díaz-Vélez, S. Flis,D. R. Williams,D. R. Nygren,T. Glüsenkamp,A. Obertacke Pollmann,B. J. Whelan, M. Schimp,S. Ter-Antonyan, K. D. Hoffman,W. Rhode,C. Spiering,René Reimann, N. Kurahashi,K. Helbing,J. L. Kelley,N. L. Strotjohann, S. Miarecki,G. S. Japaridze,S. Vanheule,K. Hultqvist,S. Wickmann,M. Kauer,L. Lu, A. Terliuk,S. De Ridder, K. Abraham,L. Brayeur,J. Madsen,K. D. de Vries,L. Mohrmann,T. Kittler,H. Taavola, M. Relich,E. Cheung,Y. Xu,T. Stanev,S. Tilav, Sho Yoshida,J. P. Yanez,S. In,L. Rädel,K. Jero, A. Olivas,J. Leuner,A. Kappes,J. P. Dumm, R. Konietz,M. Kroll,K. Becker,M. Wolf,C. Raab,H. Dujmovic,David Z. Besson,A. Keivani,V. di Lorenzo,C.-C. Fösig,M. Richman,S. Euler,Giorgio Maggi,C. Wendt,A. Ishihara,J. Lünemann, K. Holzapfel,J. L. Lanfranchi,T. Ruhe,D. Lennarz,M. Jurkovic,I. Taboada,E. Unger, M. Archinger,Thomas K. Gaisser,J. Veenkamp, S. Böser

arxiv(2016)

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摘要
IceTop is an air-shower array located on the Antarctic ice sheet at the geographic South Pole. IceTop can detect an astrophysical flux of neutrons from Galactic sources as an excess of cosmic-ray air showers arriving from the source direction. Neutrons are undeflected by the Galactic magnetic field and can typically travel 10 (E/PeV) pc before decay. Two searches are performed using 4 yr of the IceTop data set to look for a statistically significant excess of events with energies above 10 PeV (10(16) eV) arriving within a small solid angle. The all-sky search method covers from -90 degrees to approximately -50 degrees in declination. No significant excess is found. A targeted search is also performed, looking for significant correlation with candidate sources in different target sets. This search uses a higher-energy cut (100 PeV) since most target objects lie beyond 1 kpc. The target sets include pulsars with confirmed TeV energy photon fluxes and high-mass X-ray binaries. No significant correlation is found for any target set. Flux upper limits are determined for both searches, which can constrain Galactic neutron sources and production scenarios.
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astroparticle physics,cosmic rays,methods: data analysis
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