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Cosmic-muon flux and annual modulation in Borexino at 3800 m water-equivalent depth

  • G. Bellini
  • , J. Benziger
  • , D. Bick
  • , G. Bonfini
  • , D. Bravo
  • , M. Buizza Avanzini
  • , B. Caccianiga
  • , L. Cadonati
  • , F. Calaprice
  • , C. Carraro
  • , P. Cavalcante
  • , A. Chavarria
  • , A. Chepurnov
  • , D. D'Angelo
  • , S. Davini
  • , A. Derbin
  • , A. Etenko
  • , F. Von Feilitzsch
  • , K. Fomenko
  • , D. Franco
  • C. Galbiati, S. Gazzana, C. Ghiano, M. Giammarchi, M. Goeger-Neff, A. Goretti, L. Grandi, E. Guardincerri, C. Hagner, S. Hardy, Aldo Ianni, Andrea Ianni, D. Korablev, G. Korga, Y. Koshio, D. Kryn, M. Laubenstein, T. Lewke, E. Litvinovich, B. Loer, F. Lombardi, P. Lombardi, L. Ludhova, I. MacHulin, S. Manecki, W. Maneschg, G. Manuzio, Q. Meindl, E. Meroni, L. Miramonti, M. Misiaszek, D. Montanari, P. Mosteiro, V. Muratova, L. Oberauer, M. Obolensky, F. Ortica, K. Otis, M. Pallavicini, L. Papp, L. Perasso, S. Perasso, A. Pocar, R. S. Raghavan, G. Ranucci, A. Razeto, A. Re, A. Romani, A. Sabelnikov, R. Saldanha, C. Salvo, S. Schönert, H. Simgen, M. Skorokhvatov, O. Smirnov, A. Sotnikov, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, D. Vignaud, R. B. Vogelaar, J. Winter, M. Wojcik, A. Wright, M. Wurm, J. Xu, O. Zaimidoroga, S. Zavatarelli, G. Zuzel
  • University of Milano
  • Princeton University
  • Universität Hamburg
  • Laboratori Nazionali del Gran Sasso
  • Virginia Polytechnic Institute and State University
  • UMass Amherst
  • Princeton University
  • University of Genoa
  • Moscow State University
  • University of Houston
  • Petersburg Nuclear Physics Institute (PNPI)
  • Kurchatov Institute
  • Technical University of Munich
  • Joint Institute for Nuclear Research, Dubna
  • Astroparticule and Cosmol APC
  • Max-Planck-Institut für Kernphysik
  • Jagiellonian University
  • University of Perugia

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

We have measured the muon flux at the underground Gran Sasso National Laboratory (3800 m w.e.) to be (3.41±0.01)ċ10 -4m -2s -1 using four years of Borexino data. A modulation of this signal is observed with a period of (366±3) days and a relative amplitude of (1.29±0.07)%. The measured phase is (179±6) days, corresponding to a maximum on the 28 th of June. Using the most complete atmospheric data models available, muon rate fluctuations are shown to be positively correlated with atmospheric temperature, with an effective coefficient α T = 0.93±0.04. This result represents the most precise study of the muon flux modulation for this site and is in good agreement with expectations.

langue originaleAnglais
Numéro d'article015
journalJournal of Cosmology and Astroparticle Physics
Volume2012
Numéro de publication5
Les DOIs
étatPublié - 1 mai 2012
Modification externeOui

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