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Energy reconstruction methods in the IceCube neutrino telescope

  • M. G. Aartsen
  • , R. Abbasi
  • , M. Ackermann
  • , J. Adams
  • , J. A. Aguilar
  • , M. Ahlers
  • , D. Altmann
  • , C. Arguelles
  • , J. Auffenberg
  • , X. Bai
  • , M. Baker
  • , S. W. Barwick
  • , V. Baum
  • , R. Bay
  • , J. J. Beatty
  • , J. Becker Tjus
  • , K. H. Becker
  • , S. Benzvi
  • , P. Berghaus
  • , D. Berley
  • E. Bernardini, A. Bernhard, D. Z. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, J. Blumenthal, D. J. Boersma, C. Bohm, D. Bose, S. Böser, O. Botner, L. Brayeur, H. P. Bretz, A. M. Brown, R. Bruijn, J. Casey, M. Casier, D. Chirkin, A. Christov, B. Christy, K. Clark, L. Classen, F. Clevermann, S. Coenders, S. Cohen, D. F. Cowen, A. H.Cruz Silva, M. Danninger, J. Daughhetee, J. C. Davis, M. Day, C. De Clercq, S. De Ridder, P. Desiati, K. D. De Vries, M. De With, T. Deyoung, J. C. Díaz-Vélez, M. Dunkman, R. Eagan, B. Eberhardt, B. Eichmann, J. Eisch, S. Euler, P. A. Evenson, O. Fadiran, A. R. Fazely, A. Fedynitch, J. Feintzeig, T. Feusels, K. Filimonov, C. Finley, T. Fischer-Wasels, S. Flis, A. Franckowiak, K. Frantzen, T. Fuchs, T. K. Gaisser, J. Gallagher, L. Gerhardt, L. Gladstone, T. Glüsenkamp, A. Goldschmidt, G. Golup, J. G. Gonzalez, J. A. Goodman, D. Góra, D. T. Grandmont, D. Grant, P. Gretskov, J. C. Groh, A. Groß, C. Ha, A. Haj Ismail, P. Hallen, A. Hallgren, F. Halzen, K. Hanson, D. Hebecker, D. Heereman, D. Heinen, K. Helbing, R. Hellauer, S. Hickford, G. C. Hill, K. D. Hoffman, R. Hoffmann, A. Homeier, K. Hoshina, F. Huang, W. Huelsnitz, P. O. Hulth, K. Hultqvist, S. Hussain, A. Ishihara, S. Jackson, E. Jacobi, J. Jacobsen, K. Jagielski, G. S. Japaridze, K. Jero, O. Jlelati, B. Kaminsky, A. Kappes, T. Karg, A. Karle, M. Kauer, J. L. Kelley, J. Kiryluk, J. Kläs, S. R. Klein, J. H. Köhne, G. Kohnen, H. Kolanoski, L. Köpke, C. Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, M. Krasberg, A. Kriesten, K. Krings, G. Kroll, J. Kunnen, N. Kurahashi, T. Kuwabara, M. Labare, H. Landsman, M. J. Larson, M. Lesiak-Bzdak, M. Leuermann, J. Leute, J. Lünemann, O. Macías, J. Madsen, G. Maggi, R. Maruyama, K. Mase, H. S. Matis, F. Mcnally, K. Meagher, M. Merck, T. Meures, S. Miarecki, E. Middell, N. Milke, J. Miller, L. Mohrmann, T. Montaruli, R. Morse, R. Nahnhauer, U. Naumann, H. Niederhausen, S. C. Nowicki, D. R. Nygren, A. Obertacke, S. Odrowski, A. Olivas, A. Omairat, A. O'murchadha, L. Paul, J. A. Pepper, C. Pérez De Los Heros, C. Pfendner, D. Pieloth, E. Pinat, J. Posselt, P. B. Price, G. T. Przybylski, M. Quinnan, L. Rädel, M. Rameez, K. Rawlins, P. Redl, R. Reimann, E. Resconi, W. Rhode, M. Ribordy, M. Richman, B. Riedel, S. Robertson, J. P. Rodrigues, C. Rott, T. Ruhe, B. Ruzybayev, D. Ryckbosch, S. M. Saba, H. G. Sander, M. Santander, S. Sarkar, K. Schatto, F. Scheriau, T. Schmidt, M. Schmitz, S. Schoenen, S. Schöneberg, A. Schönwald, A. Schukraft, L. Schulte, O. Schulz, D. Seckel, Y. Sestayo, S. Seunarine, R. Shanidze, C. Sheremata, M. W.E. Smith, D. Soldin, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, N. A. Stanisha, A. Stasik, T. Stezelberger, R. G. Stokstad, A. Stößl, E. A. Strahler, R. Ström, N. L. Strotjohann, G. W. Sullivan, H. Taavola, I. Taboada, A. Tamburro, A. Tepe, S. Ter-Antonyan, G. Tešić, S. Tilav, P. A. Toale, M. N. Tobin, S. Toscano, M. Tselengidou, E. Unger, M. Usner, S. Van Vallecorsa, N. Van Eijndhoven, A. Van Overloop, J. Santen, M. Vehring, M. Voge, M. Vraeghe, C. Walck, T. Waldenmaier, M. Wallraff, Ch Weaver, M. Wellons, C. Wendt, S. Westerhoff, B. Whelan, N. Whitehorn, K. Wiebe, C. H. Wiebusch, D. R. Williams, H. Wissing, M. Wolf, T. R. Wood, K. Woschnagg, D. L. Xu, X. W. Xu, J. P. Yanez, G. Yodh, S. Yoshida, P. Zarzhitsky, J. Ziemann, S. Zierke, M. Zoll
  • University of Adelaide
  • University of Wisconsin-Madison
  • Deutsches Elektronen-Synchrotron (DESY)
  • University of Canterbury
  • University of Geneva
  • Friedrich Alexander Universität Erlangen-Nürnberg
  • University of Delaware
  • University of California, Irvine
  • Johannes Gutenberg University
  • University of California at Berkeley
  • Ohio State University
  • Max-Planck-lnstitut für Kohlenforschung
  • Bergische Universität Wuppertal
  • University of Maryland
  • Technical University of Munich
  • University of Kansas
  • Lawrence Berkeley National Laboratory
  • RWTH Aachen University
  • Uppsala University
  • Oskar Klein Centre
  • Sungkyunkwan University
  • University of Bonn
  • VUB Neurology
  • EPFL
  • Georgia Institute of Technology
  • University of Toronto
  • pro3dure medical GmbH
  • The Pennsylvania State University
  • Eberly College of Science
  • Ghent University
  • Humboldt-Universität zu Berlin
  • Southern University and A&M College
  • University of Alberta
  • Université Libre de Bruxelles
  • Chiba-U
  • Clark-Atlanta University
  • SUNY
  • University of Mons
  • Niels Bohr Institutet
  • Physics Dept., University of Alabama
  • University of Wisconsin-River Falls
  • University of Alaska Anchorage
  • University of Oxford

Research output: Contribution to journalArticlepeer-review

265 Scopus citations

Abstract

Accurate measurement of neutrino energies is essential to many of the scientific goals of large-volume neutrino telescopes. The fundamental observable in such detectors is the Cherenkov light produced by the transit through a medium of charged particles created in neutrino interactions. The amount of light emitted is proportional to the deposited energy, which is approximately equal to the neutrino energy for νe and νμ charged-current interactions and can be used to set a lower bound on neutrino energies and to measure neutrino spectra statistically in other channels. Here we describe methods and performance of reconstructing charged-particle energies and topologies from the observed Cherenkov light yield, including techniques to measure the energies of uncontained muon tracks, achieving average uncertainties in electromagnetic- equivalent deposited energy of ∼ 15% above 10 TeV.

Original languageEnglish
Article numberP03009
JournalJournal of Instrumentation
Volume9
Issue number3
DOIs
StatePublished - Mar 2014

Keywords

  • Cherenkov detectors
  • Neutrino detectors
  • Performance of High Energy Physics Detectors
  • dE/dx detectors

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