Evidence for correlated changes in the spectrum and composition of cosmic rays at extremely high energies

D. J. Bird, S. C. Corbató, H. Y. Dai, B. R. Dawson, J. W. Elbert, T. K. Gaisser, K. D. Green, M. A. Huang, D. B. Kieda, S. Ko, C. G. Larsen, E. C. Loh, M. Luo, M. H. Salamon, D. Smith, P. Sokolsky, P. Sommers, T. Stanev, J. K. K. Tang, S. B. Thomas, and S. Tilav
Phys. Rev. Lett. 71, 3401 – Published 22 November 1993
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Abstract

The Utah Fly’s Eye detector has revealed a change in the cosmic ray composition which is correlated with structure in the all-particle energy spectrum. The data can be fitted by a simple model of a steep power law spectrum of heavy nuclei which is overtaken at high energies by a flatter spectrum of protons. The transition occurs near 1018.5 eV. Anisotropy is not detected, so the high-rigidity particles above the transition energy do not originate in the disk of the Galaxy. An outstanding event of 3×1020 eV implies that the highest energy particles originate in the contemporary era of the Universe.

  • Received 14 September 1993

DOI:https://doi.org/10.1103/PhysRevLett.71.3401

©1993 American Physical Society

Authors & Affiliations

D. J. Bird, S. C. Corbató, H. Y. Dai, B. R. Dawson, J. W. Elbert, T. K. Gaisser, K. D. Green, M. A. Huang, D. B. Kieda, S. Ko, C. G. Larsen, E. C. Loh, M. Luo, M. H. Salamon, D. Smith, P. Sokolsky, P. Sommers, T. Stanev, J. K. K. Tang, S. B. Thomas, and S. Tilav

  • Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801
  • Department of Physics and Mathematical Physics, University of Adelaide, Adelaide, South Australia 5005, Australia
  • High Energy Astrophysics Institute, Department of Physics, University of Utah, Salt Lake City, Utah 84112
  • Bartol Research Institute, University of Delaware, Newark, Delaware 19716

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Vol. 71, Iss. 21 — 22 November 1993

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