Photons as carriers of ultra-high energy in cosmic space
Journal of Samara State Technical University, Ser. Physical and Mathematical Sciences, no. 2 (2013), pp. 228-232.

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Absorbing process of ultrahigh-energy gamma-quanta in a cosmic space is investigated. It is shown that the main absorbing mechanism is the reactions arising at collisions of cosmic-ray photons with microwave and radio background ones. Estimate of the mean free path of a photon for different energies gives evidence that gamma-quanta with energies $E > 10^{19}$ eV running from Active Galactic Nuclei seem to reach the Earth vicinity. This result is in agreement with the recent observations of extensive air shower array experiments realized by AGASA and Yakutsk.
Keywords: cosmic rays
Mots-clés : ultrahigh-energy photons.
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E. A. Buyanova; L. S. Molchatsky. Photons as carriers of  ultra-high energy in cosmic space. Journal of Samara State Technical University, Ser. Physical and Mathematical Sciences, no. 2 (2013), pp. 228-232. http://geodesic.mathdoc.fr/item/VSGTU_2013_2_a26/

[1] V. L. Ginzburg, “What problems of physics and astrophysics seem now to be especially important and interesting (thirty years later, already on the verge of XXI century)?”, Phys. Usp., 42:4 (1999), 353–373 | DOI | DOI

[2] K. Greisen, “End to the Cosmic-Ray Spectrum?”, Phys. Rev. Lett., 16:17 (1966), 748–750 | DOI

[3] G. T. Zatsepin, V. A. Kuz'min, “Upper Limit of the Spectrum of Cosmic Rays”, JETP Letters, 4:3, 78–80

[4] V. S. Berezinskii, S. V. Bulanov, V. A. Dogiel, V. L. Ginzburg, V. S. Ptuskin, Astrophysics of Cosmic Rays, North-Holland, Amsterdam, 1990, xii+534 pp.

[5] J. W. Elbert, P. Somers, “In search of a source for the 320 EeV Fly's Eye cosmic ray”, Astroph. J., 441:1 (1995), 151–161, arXiv: astro-ph/9410069 | DOI

[6] A. V. Glushkov, I. T. Makarov, M. I. Pravdin, I. E. Sleptsov, D. S. Gorbunov, G. I. Rubtsov, S. V. Troitsky, “Constraints on the flux of primary cosmic-ray photons at energies ${E>10^{18}}$ eV from Yakutsk muon data”, Phys. Rev. D, 82:4 (2010), 041101(R), 5 pp., arXiv: [astro-ph.HE] 0907.0374 | DOI

[7] M. Risse, P. Homola, R. Engel, D. Góra, D. Heck, J. Pekala, B. Wilczyńska, H. Wilczyński, “Upper limit on the photon fraction in highest-energy cosmic rays from AGASA data”, Phys. Rev. Lett., 95:17 (2005), 171102, 4 pp. | DOI

[8] G. I. Rubtsov, L. G. Dedenko, G. F. Fedorova, E. Yu. Fedunin, A. V. Glushkov, D. S. Gorbunov, I. T. Makarov, M. I. Pravdin, T. M. Roganova, I. E. Sleptsov, S. V. Troitsky, “Upper limit on the ultrahigh-energy photon flux from AGASA and Yakutsk data”, Phys. Rev. D, 73:6 (2006), 063009, 8 pp., arXiv: astro-ph/0601449 | DOI

[9] V. A. Ryabov, “Ultrahigh-energy neutrinos from astrophysical sources and superheavy particle decays”, Phys. Usp., 49:9 (2006), 905–936 | DOI | DOI

[10] A. D. Filonenko, “Radioastronomical measurement of ultrahigh-energy cosmic particle fluxes”, Phys. Usp., 55:8 (2012), 741–772 | DOI | DOI