Abstract
The complicated form of the cosmic-ray spectrum recorded in the energy range 1017–1020 eV by giant detector arrays is analyzed. It is shown that the spectrum in the region 1018–1019 eV is apparently identical to the injection spectrum with power-law exponent approximately equal to 3.2–3.3. The flat component in the region (3.2–5)×1019 eV is due to the braking of extragalactic protons by relict photons. The spectrum apparently has no blackbody cutoff at energies above 3.2×1019 eV.
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References
V. S. Berezinskii, S. V. Bulanov, V. L. Ginzburg et al., The Astrophysics of Cosmic Rays [in Russian], Nauka, Moscow, 1990.
M. N. D’yakonov, T. A. Egorov, N. N. Efimov et al., Ultra-High-Energy Cosmic Rays [in Russian], Nauka, Novosibirsk, 1991.
M. Teshima, in Proc. 23rd ICRC, Calgary. Invited, Rapporteur and Highlight Papers, edited by D. A. Leakhy, R. B. Hicks, and D. Venkatesan, World Scientific, New York, 1993, p. 257.
G. T. Zatsepin and V. A. Kuz’min, JETP Lett. 4, 78 (1966).
K. Greisen, Phys. Rev. Lett. 16, 748 (1966).
F. W. Stecker, Phys. Rev. Lett. 21, 1016 (1968).
A. V. Uryson, JETP Lett. 64, 77 (1996).
B. N. Afanasiev, M. N. Dyakonov, T. A. Egorov et al. in Proc. 24th ICRC, Rome (1995), Vol. 2, p. 756.
M. Nagano et al. J. Phys. G: Nucl. Phys. 18, 423 (1992).
O. J. Bird, S. C. Corbato, H. Y. Dai et al., Astrophys. J. 424, 491 (1994).
M. A. Lawrence, R. J. O. Reid, and A. A. Watson, J. Phys. G: Nucl. Phys. 17, 733 (1991).
M. M. Winn, J. Ulrichs, L. S. Deak et al., J. Phys. G: Nucl. Phys. 12, 653 (1986).
J. Linsley, G. Cunningam, D. M. Edge et al., Catalogue of Highest Energy Cosmic Rays, N1, World Data Center C2, Japan, 1980.
V. S. Ptuskin, S. I. Rogovaya, V. N. Zirakashvili et al., Astron. Astrophys. 268, 726 (1993).
S. I. Syrovatskii, Comments Astrophys. Space Phys. 3, 155 (1971).
V. S. Berezinsky, A. A. Mikhailov, and S. I. Syrovatskii, Proc. 16th ICRC, Kyoto (1979), Vol. 2, p. 86.
V. A. Dogiel, A. V. Gurevich, and K. P. Zybin, Astron. Astrophys. 281, 937 (1994).
M. N. D’yakonov, V. P. Egorova, A. A. Ivanov et al., JETP Lett. 50, 442 (1989).
J. Rachen, T. Stanev, and P. Biermann, Astron. Astrophys. 273, 377 (1995).
R. J. Protheroe and P. A. Johnson, Proc. 24th ICRC, Rome (1995), Vol. 3, p. 309.
A. M. Hillas, Can. J. Phys. 21, 1016 (1968).
C. T. Hill and D. N. Schramm, Phys. Rev. D 31, 564 (1985).
V. S. Berezinskii and S. I. Grigor’eva, Zh. Éksp. Teor. Fiz. 93, 812 (1987) [Sov. Phys. JETP 66, 457 (1987)].
D. N. Pochepkin, V. S. Ptuskin, S. I. Rogovaya et al., Proc. 24th ICRC, Rome, 3, 136 (1995).
M. Teshima et al., Nucl. Phys. B, Proc. Suppl. 28, 169 (1992).
J. W. Cronin, Nucl. Phys. A 25, 137 (1992).
S. S. Ameev, I. Y. Chasnikov, Yu. A. Fomin et al., Proc. 24th ICRC, Rome (1995), Vol. 1, p. 466.
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Pis’ma Zh. Éksp. Teor. Fiz. 65, No. 10, 729–733 (25 May 1997)
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Uryson, A.V. Possible origin and spectrum of ultrahigh-energy cosmic rays. Jetp Lett. 65, 763–767 (1997). https://doi.org/10.1134/1.567423
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DOI: https://doi.org/10.1134/1.567423