Phys. Rev. Lett.
100,
101101
(2008)
[5 pages]
First Observation of the Greisen-Zatsepin-Kuzmin Suppression
R. U. Abbasi et al. High Resolution Fly’s Eye Collaboration
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R. U. Abbasi1, T. Abu-Zayyad1, M. Allen1, J. F. Amman2, G. Archbold1, K. Belov1, J. W. Belz1, S. Y. Ben Zvi3, D. R. Bergman4,*, S. A. Blake1, O. A. Brusova1, G. W. Burt1, C. Cannon1, Z. Cao1, B. C. Connolly3, W. Deng1, Y. Fedorova1, C. B. Finley3, R. C. Gray1, W. F. Hanlon1, C. M. Hoffman2, M. H. Holzscheiter2, G. Hughes4, P. Hüntemeyer1, B. F Jones1, C. C. H. Jui1, K. Kim1, M. A. Kirn5, E. C. Loh1, M. M. Maestas1, N. Manago6, L. J. Marek2, K. Martens1, J. A. J. Matthews7, J. N. Matthews1, S. A. Moore1, A. O’Neill3, C. A. Painter2, L. Perera4, K. Reil1, R. Riehle1, M. Roberts7, D. Rodriguez1, N. Sasaki6, S. R. Schnetzer4, L. M. Scott4, G. Sinnis2, J. D. Smith1, P. Sokolsky1, C. Song3, R. W. Springer1, B. T. Stokes1, S. B. Thomas1, J. R. Thomas1, G. B. Thomson4, D. Tupa2, S. Westerhoff3, L. R. Wiencke1, X. Zhang3, and A. Zech4 (High Resolution Fly’s Eye Collaboration)
1Department of Physics, University of Utah, Salt Lake City, Utah 84112, USA 2Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA 3Department of Physics and Nevis Laboratory, Columbia University, New York, New York 10027, USA 4Department of Physics and Astronomy, Rutgers University—The State University of New Jersey, Piscataway, New Jersey 08854, USA 5Department of Physics, Montana State University, Bozeman, Montana 59717, USA 6Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan 7Department of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico 87131, USA
Received 5 March 2007; revised 7 January 2008; published 10 March 2008
The High Resolution Fly’s Eye (HiRes) experiment has observed the Greisen-Zatsepin-Kuzmin suppression (called the GZK cutoff) with a statistical significance of five standard deviations. HiRes’ measurement of the flux of ultrahigh energy cosmic rays shows a sharp suppression at an energy of 6×1019 eV, consistent with the expected cutoff energy. We observe the ankle of the cosmic-ray energy spectrum as well, at an energy of 4×1018 eV. We describe the experiment, data collection, and analysis and estimate the systematic uncertainties. The results are presented and the calculation of the statistical significance of our observation is described.
© 2008 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevLett.100.101101
DOI:
10.1103/PhysRevLett.100.101101
PACS:
98.70.Sa, 95.85.Ry, 96.50.sb, 96.50.sd
*Corresponding author. bergman@physics.rutgers.edu
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