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Volumn 59, Issue 9, 1999, Pages

Hadronic interaction models beyond collider energies

Author keywords

[No Author keywords available]

Indexed keywords


EID: 85037916808     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.59.094003     Document Type: Article
Times cited : (40)

References (35)
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  • 4
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    • Phys. Rev. Lett.M. Takeda, 81, 1163 (1998)] became a challenge to current models for the production of cosmic rays because of the predicted cutoff in the energy spectrum;
    • (1998) Phys. Rev. Lett. , vol.81 , pp. 1163
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    • UA1 Collaboration, C. Albajar, Nucl. Phys. B309, 405 (1988).
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    • UA1 Collaboration, G. Arnison, Phys. Lett. 118B, 167 (1982).
    • (1982) Phys. Lett. , vol.118B , pp. 167
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    • Details on hadron-nucleus interactions as described by QGSJET are discussed in A. B. Kaidalov, K. A. Ter-Martirosyan, and Yu. M. Shabel’skii, Yad. Fiz. 43, 1282 (1986) [Sov. J. Nucl. Phys. 43, 822 (1986)].
    • (1986) Sov. J. Nucl. Phys. , vol.43 , pp. 822
    • Kaidalov, A.B.1    Ter-Martirosyan, K.A.2
  • 20
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    • Report FZKA 5828 (1996);
    • A comparison of hadronic interaction models used in air shower simulations have been already performed by the group of Karlsruhe with the code CORSIKA. The analysis was based on proton and iron induced showers with primaries energies ranging from (Formula presented) to (Formula presented) See, J. Knapp, D. Heck, and G. Schatz, Nucl. Phys. B (Proc. Suppl.) 52B, 136 (1997);Report FZKA 5828 (1996);
    • (1997) Nucl. Phys. B (Proc. Suppl.) , vol.52B , pp. 136
    • Knapp, J.1    Heck, D.2    Schatz, G.3
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    • hep-ph/9809588
    • See also G. Battistoni, hep-ph/9809588.
    • Battistoni, G.1
  • 23
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    • S. J. Sciutto, “AIRES: A System for Air Shower Simulations,” Auger technical note GAP-98-032 (1998); available electronically from http://www-td-auger.fnal.gov:82
    • S. J. Sciutto, “AIRES: A System for Air Shower Simulations,” Auger technical note GAP-98-032 (1998); available electronically from http://www-td-auger.fnal.gov:82
  • 24
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    • Most of the electromagnetic algorithms are based on the well known MOCCA simulation program by A. M. Hillas, Nucl. Phys. B (Proc. Suppl.) 52, 29 (1997).
    • (1997) Nucl. Phys. B (Proc. Suppl.) , vol.52 , pp. 29
    • Hillas, A.M.1
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    • See
    • T. Hara, Phys. Rev. Lett. 50, 2058 (1983). It is important to stress that while computing these data an energy dependence on (Formula presented) represented as (Formula presented) was taken into account. This parametrization was obtained with the assumption that there is no significant break of Feynman scaling in the fragmentation region and that the multiplicity increases as (Formula presented) The value of (Formula presented) is expected to become a little smaller if there is a significant breakdown of scaling in the fragmentation region.See 19.
    • (1983) Phys. Rev. Lett. , vol.50 , pp. 2058
    • Hara, T.1
  • 30
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    • see also SIBYLL source code.
    • T. K. Gaisser (private communication);see also SIBYLL source code.
    • Gaisser, T.K.1
  • 31
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    • updated in Procedings of the 17th International Cosmic Ray Conference, Paris, France, 1981 (CEN, Saclay, 1981), Vol. 8, p. 183.
    • A. M. Hillas, in Proceedings of the 16th International Cosmic Ray Conference, Tokyo, Japan, 1979 (University of Tokyo, Tokyo, 1979), Vol. 8, p. 7;updated in Procedings of the 17th International Cosmic Ray Conference, Paris, France, 1981 (CEN, Saclay, 1981), Vol. 8, p. 183.
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  • 32
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    • C. Pryke and L. Voyvodick, Proceedings of the 10th International Symposium on Very High Energy Cosmic Ray Interactions, 1998 (LNGS, Assergi, Italy, in press);, Auger technical note GAP-98-052 (1998), available electronically from: http://www-td-auger.fnal.gov:82
    • C. Pryke and L. Voyvodick, Proceedings of the 10th International Symposium on Very High Energy Cosmic Ray Interactions, 1998 (LNGS, Assergi, Italy, in press);Auger technical note GAP-98-052 (1998), available electronically from: http://www-td-auger.fnal.gov:82
  • 34
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    • The Auger Collaboration, Pierre Auger Project Design Report, Fermi National Accelerator Laboratory, available electronically from http://www-td-auger-fnal.gov:82
    • The Auger Collaboration, Pierre Auger Project Design Report, Fermi National Accelerator Laboratory, available electronically from http://www-td-auger-fnal.gov:82


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