Abstract
At high energy, cosmic rays can only be studied by measuring the extensive air showers they produce in the atmosphere of the Earth. Although the main features of air showers can be understood within a simple model of successive interactions, detailed simulations and a realistic description of particle production are needed to calculate observables relevant to air shower experiments. Currently hadronic interaction models are the main source of uncertainty of such simulations. We will study the effect of using different hadronic models available in corsika and conex on extensive air shower predictions.
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References
J. Abraham et al. [Pierre Auger Collaboration]: Nucl. Instrum. Meth. A 523 (2004) 50.
J. Knapp, D. Heck, and G. Schatz: Report FZKA 5828 (1996).
J. Knapp et al.: Astropart. Phys., 19 (2003) 77.
W. Heitler, The Quantum Theory of Radiation, third ed., Oxford University Press, London, 1954, p. 386.
D. Heck et al.: Report FZKA 6019 (1998), Forschungszentrum Karlsruhe.
T. Pierog et al.: Nucl. Phys. B (Proc. Suppl.) 151 (2006) 159
R. Engel: Nucl. Phys. B (Proc. Suppl.) 122 (2003) 40.
S. S. Ostapchenko: J. Phys. G29 (2003) 831.
M. Zha, J. Knapp, and S. Ostapchenko: Proc. 28th Int. Cosmic Ray Conf. (ICRC 2003), Tsukuba (Japan) (2003) 515.
S. S. Ostapchenko: These proceedings, Prague (Czech. Rep.) (2005), [arXiv:hepph/ 0601230].
J. Matthews: Astropart. Phys. 22 (2005) 387.
C. Meurer et al.: These proceedings, Prague (Czech. Rep.) (2005), [arXiv:astroph/ 0512536].
J. Alvarez-Muniz et al.: Phys. Rev. D66 (2002) 033011.
J. Ranft: Phys. Rev. D51 (1995) 64.
H. J. Drescher et al.: Phys. Rept. 350 (2001) 93.
T. Pierog et al.: Nucl. Phys. A71 (2003) 895–898.
N.N. Kalmykov et al.: Nucl. Phys. B (Proc. Suppl.) 52B (1997) 17.
S. Ostapchenko: Nucl. Phys. B (Proc. Suppl) 151 (2006) 143.
S. Ostapchenko: [arXiv:hep-ph/0501093] (2005).
R. S. Fletcher et al.: Phys. Rev. D50 (1994) 5710.
J. Engel et al.: Phys. Rev. D46 (1992) 5013.
R. Engel et al.: Proc. 26th Int. Cosmic Ray Conf., Salt Lake City (USA), 1 (1999) 415.
R. Engel and H. Rebel: Acta Phys. Polon. B 35 (2004) 321.
A. Fassò et al.: FLUKA: Status and Prospective of Hadronic Applications, (Proc. Monte Carlo 2000 Conf., Lisbon, Oct. 23–26, 2000) (A. Kling, F. Barao, M. Nakagawa, P. Vaz eds.), Springer, Berlin, 2001, 955.
H. Fesefeldt: Report PITHA-85/02 (1985), RWTH Aachen.
S.A. Bass et al.: Prog. Part. Nucl. Phys. 41 (1998) 225; M. Bleicher et al.: J. Phys. G: Nucl. Part. Phys. 25 (1999) 1859.
H.-J. Drescher et al., Astropart. Phys. 21 (2004) 87.
D. Heck: Nucl. Phys. B (Proc. Suppl.) 151 (2006) 127.
T. Pierog et al.: Proc. 29th Int. Cosmic Ray Conf., Pune, India (2005).
R. Engel and H. Klages: Comptes Rendus Physique 5 (2004) 505.
H. Ulrich: These proceedings, Prague (Czech. Rep.) (2005).
A. M. Hillas: Proc. 11th Int. Cosmic Ray Conf., Budapest (1969) 355.
C. Pajares, D. Sousa, and R. A. Vazquez: Phys. Rev. Lett. 86 (2001) 1674.
H. J. Drescher, A. Dumitru, and M. Strikman, Phys. Rev. Lett. 94 (2005) 231801.
J. Dias de Deus et al.: [arXiv:hep-ph/0507227] (2005).
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Pierog, T., Engel, R. & Heck, D. Impact of uncertainties in hadron production on air-shower predictions. Czech J Phys 56 (Suppl 1), A161–A172 (2006). https://doi.org/10.1007/s10582-006-0152-0
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DOI: https://doi.org/10.1007/s10582-006-0152-0