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Searches for relativistic magnetic monopoles in IceCubeopen access

Authors
Aartsen, M.G.Abraham, K.Ackermann, M.Adams, J.Aguilar, J.A.Ahlers, M.Ahrens, M.Altmann, D.Anderson, T.Ansseau, I.Archinger, M.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.Beiser, E.Benabderrahmane, M.L.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.Börner, M.Bos, F.Bose, D.Böser, S.Botner, O.Braun, J.Brayeur, L.Bretz, H.-P.Buzinsky, N.Casey, J.Casier, M.Cheung, E.Chirkin, D.Christov, A.Clark, K.Classen, L.Coenders, S.Cowen, D.F.Cruz Silva, A.H.Daughhetee, J.Davis, J.C.Day, M.de, André J.P.A.M.De, Clercq C.del, Pino Rosendo E.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.Dumm, J.P.Dunkman, M.Eberhardt, B.Ehrhardt, T.Eichmann, B.Euler, S.Evenson, P.A.Fahey, S.Fazely, A.R.Feintzeig, J.Felde, J.Filimonov, K.Finley, C.Fischer-Wasels, T.Flis, S.Fösig, C.-C.Fuchs, T.Gaisser, T.K.Gaior, R.Gallagher, J.Gerhardt, L.Ghorbani, K.Gier, D.Gladstone, L.Glagla, M.Glüsenkamp, T.Goldschmidt, A.Golup, G.Gonzalez, J.G.Góra, D.Grant, D.Griffith, Z.Groß, A.Ha, C.Haack, C.Haj, Ismail A.Hallgren, A.Halzen, F.Hansen, E.Hansmann, B.Hanson, K.Hebecker, D.Heereman, D.Helbing, K.Hellauer, R.Hickford, S.Hignight, J.Hill, G.C.Hoffman, K.D.Hoffmann, R.Holzapfel, K.Homeier, A.Hoshina, K.Huang, F.Huber, M.Huelsnitz, W.Hulth, P.O.Hultqvist, K.In, S.Ishihara, A.Jacobi, E.Japaridze, G.S.Jeong, M.Jero, K.Jurkovic, M.Kappes, A.Karg, T.Karle, A.Kauer, M.Keivani, A.Kelley, J.L.Kemp, J.Kheirandish, A.Kiryluk, J.Kläs, J.Klein, S.R.Kohnen, G.Koirala, R.Kolanoski, H.Konietz, R.Köpke, L.Kopper, C.Kopper, S.Koskinen, D.J.Kowalski, M.Krings, K.Kroll, G.Kroll, M.Krückl, G.Kunnen, J.Kurahashi, N.Kuwabara, T.Labare, M.Lanfranchi, J.L.Larson, M.J.Lesiak-Bzdak, M.Leuermann, M.Leuner, J.Lu, L.Lünemann, J.Madsen, J.Maggi, G.Mahn, K.B.M.Mandelartz, M.Maruyama, R.Mase, K.Matis, H.S.Maunu, R.McNally, F.Meagher, K.Medici, M.Meli, A.Menne, T.Merino, G.Meures, T.Miarecki, S.Middell, E.Mohrmann, L.Montaruli, T.Morse, R.Nahnhauer, R.Naumann, U.Neer, G.Niederhausen, H.Nowicki, S.C.Nygren, D.R.Obertacke, Pollmann A.Olivas, A.Omairat, A.O’Murchadha, A.Palczewski, T.Pandya, H.Pankova, D.V.Paul, L.Pepper, J.A.Pérez, de los Heros C.Pfendner, C.Pieloth, D.Pinat, E.Posselt, J.Price, P.B.Przybylski, G.T.Pütz, J.Quinnan, M.Raab, C.Rädel, L.Rameez, M.Rawlins, K.Reimann, R.Relich, M.Resconi, E.Rhode, W.Richman, M.Richter, S.Riedel, B.Robertson, S.Rongen, M.Rott, C.Ruhe, T.Ryckbosch, D.Sabbatini, L.Sander, H.-G.Sandrock, A.Sandroos, J.Sarkar, S.Schatto, K.Scheriau, F.Schimp, M.Schmidt, T.Schmitz, M.Schoenen, S.Schöneberg, S.Schönwald, A.Schulte, L.Schumacher, L.Seckel, D.Seunarine, S.Soldin, D.Song, M.Spiczak, G.M.Spiering, C.Stahlberg, M.Stamatikos, M.Stanev, T.Stasik, A.Steuer, A.Stezelberger, T.Stokstad, R.G.Stößl, A.Ström, R.Strotjohann, N.L.Sullivan, G.W.Sutherland, M.Taavola, H.Taboada, I.Tatar, J.Ter-Antonyan, S.Terliuk, A.Tešić, G.Tilav, S.Toale, P.A.Tobin, M.N.Toscano, S.Tosi, D.Tselengidou, M.Turcati, A.Unger, E.Usner, M.Vallecorsa, S.Vandenbroucke, J.van, Eijndhoven N.Vanheule, S.van, Santen J.Veenkamp, J.Vehring, M.Voge, M.Vraeghe, M.Walck, C.Wallace, A.Wallraff, M.Wandkowsky, N.Weaver, C.Wendt, C.Westerhoff, S.Whelan, B.J.Wiebe, K.Wiebusch, C.H.Wille, L.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.Zoll, M.IceCube Collaboration
Issue Date
Mar-2016
Publisher
Springer New York LLC
Citation
European Physical Journal C, v.76, no.3
Journal Title
European Physical Journal C
Volume
76
Number
3
URI
https://scholarworks.bwise.kr/cau/handle/2019.sw.cau/64295
DOI
10.1140/epjc/s10052-016-3953-8
ISSN
1434-6044
1434-6052
Abstract
Various extensions of the Standard Model motivate the existence of stable magnetic monopoles that could have been created during an early high-energy epoch of the Universe. These primordial magnetic monopoles would be gradually accelerated by cosmic magnetic fields and could reach high velocities that make them visible in Cherenkov detectors such as IceCube. Equivalently to electrically charged particles, magnetic monopoles produce direct and indirect Cherenkov light while traversing through matter at relativistic velocities. This paper describes searches for relativistic ((Formula presented.)) and mildly relativistic ((Formula presented.)) monopoles, each using one year of data taken in 2008/2009 and 2011/2012, respectively. No monopole candidate was detected. For a velocity above (Formula presented.) the monopole flux is constrained down to a level of (Formula presented.). This is an improvement of almost two orders of magnitude over previous limits. © 2016, The Author(s).
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자연과학대학 (물리학과)
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