Abstract
We review all existing air-fluorescence measurements of the elongation rate of extensive air showers (slope of mean EAS shower maximum Xmax vs. log of shower energy E) above 1017 eV. We find remarkable agreement for all current and historic experiments over a 30 yr period for the energy range from 1017 to 3 × 1018 eV. The mean elongation rate in this energy interval is near 80 g/cm2/decade. Above this energy, experiments in the Northern hemisphere are in good agreement with an average elongation rate of 48 ± 10 g/cm2/decade while Southern hemisphere experiments have a flatter elongation rate of 26 ± 2 g/cm2/decade. We point out that, given the agreement at lower energies, possible systematic reasons for this difference are unlikely. Given this, the world elongation rate data alone may indicate a composition difference of UHECR in the Northern and Southern hemisphere and thus a diversity of UHECR sources in the Northern and Southern sky.
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REFERENCES
K. Greisen, Ann. Rev. Nucl. Sci 10, 63 (1960);
J. Delvaille, F. Kendziorski, and K. Greisen, J. Phys. Soc. Jpn. 17 (Suppl. A-III), 76 (1962);
K. Suga, in Proceedings of the 5th Interamerican Seminar on Cosmic Rays, La Paz, Bolivia (1962), Vol. 2, XLIX; A. E. Chudakov, in Proceedings of the 5th Interamerican Seminar on Cosmic Rays, La Paz, Bolivia (1962), Vol. 2, XLIX.
G. L. Cassiday, R. Cooper, S. Corbato, et al., Astrophys. J. 356, 669 (1990).
J. Linsley, in Proceedings of the 15th International Cosmic Rays Conference, Plovdiv, Bulgaria (1977), Vol. 8, p. 353.
D. J. Bird, S. C. Corbato, H. Y. Dai, et al., Phys. Rev. Lett. 71, 3401 (1993).
R. M. Baltrusaitis, G. L. Cassiday, R. Cooper, et al., Nucl. Instrum. Methods Phys. Res., Sect. A 240, 410 (1985).
J. M. Matthews, in Proceedings of the 27th International Cosmic Rays Conference (2001);
R. U. Abbasi, T. Abu-Zayyad, J. F. Aman, et al., Phys. Rev. Lett. 92, 151101 (2004).
T. Abu-Zayyad, K. Belov, J. Boyer, et al., Nucl. Instrum. Methods Phys. Res., Sect. A 450, 253 (2000);
T. Abu-Zayyad, K. Belov, D. J. Bird, et al., Astrophys. J. 557 (2001);
A. Borione, C. E. Couvault, J. W. Cronin, et al., Nucl. Instrum. Methods Phys. Res. 346, 329 (1994).
K. Martens, Nucl. Phys. B Proc. Suppl., 165 (2007).
H. Shin, in Proceedings of 2021 International Cosmic Ray Conference ICRC, Berlin, PoS (ICRC2021), 305 (2021).
R. U. Abbasi, T. Abu-Zayyad, M. Allen, et al., Astrophys. J. 909, 178 (2021).
K. Fujita, in Proceedings of 2021 International Cosmic Ray Conference ICRC, Berlin, PoS (ICRC2021), 353 (2021).
R. U. Abbasi, M. Abe, T. Abu-Zayyad, et al., Astropart. Phys. 64, 49 (2015).
R. U. Abbasi, T. Abu-Zayyad, G. Archbold, et al., Astrophys. J. 622, 910 (2005).
R. U. Abbasi, M. Abe, T. Abu-Zayyad, et al., Astrophys. J. 858, 76 (2018).
A. Aab, P. Abreu, M. Aglietta, et al., Nucl. Instrum. Methods Phys. Res., Sect. A 798, 172 (2015).
A. Aab, P. Abreu, M. Aglietta, et al., Phys. Rev. D 90, 122005 (2014).
V. de Souza, in Proceedings of 2017 International Cosmic Ray Conference ICRC, Beijing, China, PoS (ICRC2017), 301 (2017).
A. Watson, in Proceedings of UHECR 2018, EPJ Web of Conf. 210 (2019). https://doi.org/10.1051/epjconf/201921000001
A. di Matteo, in Proceedings of 2021 International Cosmic Ray Conference ICRC, Berlin, PoS (ICRC2021), 308 (2021).
K. Kawata, A. di Matteo, T. Fujii, et al., in Proceedings of 2019 International Cosmic Ray Conference ICRC, Madison, USA, PoS (ICRC2019), 310 (2019);
T. Fujii, D. Ivanov, C. C. H. Jui, et al., in Proceedings of 2021 International Cosmic Ray Conference ICRC, Berlin, Pos (ICRC2021), 392 (2021).
V. A. Belayev and A. E. Chudakov, Bull. USSR Acad. Sci., Phys. Ser. 30, 1700 (1966).
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Sokolsky, P., D’Avignon, R. The Unreasonable Effectiveness of the Air-Fluorescence Technique in Determining the EAS Shower Maximum. J. Exp. Theor. Phys. 134, 459–468 (2022). https://doi.org/10.1134/S1063776122040100
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DOI: https://doi.org/10.1134/S1063776122040100