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Science

Vol 9 No 2 (2024): December

EAS Cherenkov LDF Analysis: CORSIKA Simulations for Tunka-133 and Chacaltaya Arrays



(*) Corresponding Author
DOI
https://doi.org/10.21070/acopen.9.2024.8376
Published
December 28, 2023

Abstract

This study leverages CORSIKA simulations to analyze the Lateral Distribution Function (LDF) of Cherenkov photons in Extensive Air Showers (EAS) within the knee region of the cosmic ray energy spectrum (10^15 - 10^16 eV). Focusing on primary particles like helium, proton, oxygen, and iron nuclei at varying zenith angles (0˚, 20˚, and 45˚), we aimed to reconstruct Cherenkov photons' LDF using an Exponential Function model, tailored as a function of primary energy. Our approach involved a comparative analysis of simulated LDFs with experimental data from the Tunka-133 and Chacaltaya arrays. The results exhibit a high degree of concordance between simulated and observed data, affirming the validity of our method. We developed a set of approximation functions for different primary particles and zenith angles, enhancing our ability to identify the particle type in EAS events and accurately determine its energy. The primary contribution of our work lies in its potential to rapidly compile a comprehensive LDF pattern library, instrumental for analyzing real EAS array events and reconstructing the mass composition and primary cosmic ray energy spectrum. This advancement in CORSIKA-based simulation methods marks a significant stride in cosmic ray research, offering a robust tool for detailed EAS analysis.

Highlights : 

  • Validation of Simulation Accuracy: Demonstrated high concordance between CORSIKA simulated LDFs and experimental data from Tunka-133 and Chacaltaya arrays.
  • Enhanced Particle Identification: Development of approximation functions for various primary particles and zenith angles, improving accuracy in identifying particle types in EAS events.
  • Advancement in Cosmic Ray Research: Potential to create a comprehensive LDF pattern library, significantly aiding in the reconstruction of mass composition and primary cosmic ray energy spectrum.
 

Keywords : CORSIKA Simulations, Cherenkov LDF, EAS Analysis, Cosmic Ray Spectrum, Particle Identification

References

  1. G. Krymsky, “A regular mechanism for the acceleration of charged particles on the front of a shock wave,” Doklady Akademii Nauk USSR, vol. 234, pp. 1306–1308, 1977.
  2. K. F. Fadhel and A. A. Al-Rubaiee, "Reconstruction of Air-Shower Parameters Through the Lateral Distribution Function of Ultra-High Energy Particles," arXiv preprint arXiv:2201.01368, 2022.
  3. M. Brankova, A. Mishev, and J. Stamenov, "Il Nuovo Cimento C," vol. 24, pp. 525-530.
  4. J.W. Fowler et al., “A measurement of the cosmic ray spectrum and composition at the knee,” Astroparticle Physics, vol. 15, no. 1, pp. 49-64, 2001.
  5. A. Mishev, "Analysis of Lateral Distribution of Atmospheric Cherenkov Light at High Mountain Altitude Towards Event Reconstruction," vol. 2012, Article ID 906358, 12 pages, 2012.
  6. A. R. Bell, "Cosmic ray acceleration," Astroparticle Physics, vol. 43, pp. 56-70, 2013.
  7. W. Galbraith and J. V. Jelley, “Light pulses from the night sky associated with cosmic rays,” Nature, vol. 171, no. 4347, pp. 349–350, 1953.
  8. A. A. Al-Rubaiee et al., “Modeling and parameterization of the spatial distribution of Cerenkov light from extensive air showers,” Russian Physics Journal, vol. 48, no. 10, pp. 1004–1011, 2005.
  9. G. Agnetta et al., “Extensive air showers and diffused Cherenkov light detection: The ULTRA experiment,” Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 570, pp. 22–35, 2007.
  10. N. Akchurin et al., “Comparison of high-energy electromagnetic shower profiles measured with scintillation and Cherenkov light,” Nuclear Instruments and Methods in Physics Research A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 548, no. 3, pp. 336–354, 2005.
  11. W. Galbraith and J. V. Jelley, “Light pulses from the night sky associated with cosmic rays,” Nature, vol. 171, no. 4347, pp. 349–350, 1953.
  12. G. Vacanti et al., “Gamma-ray observations of the Crab Nebula at TeV energies,” Astrophysical Journal Letters, vol. 377, no. 2, pp. 467–479, 1991.
  13. T. Weekes, “Very high energy gamma-ray astronomy,” Physics Reports, vol. 160, no. 1-2, pp. 1–121, 1988.
  14. V.V. Prosin et al., "Primary CR energy spectrum and mass composition by the data of Tunka-133 array," Conferences, vol. 99, 04002, 2015.
  15. Y. Tsunesada et al., “A Cherenkov light detection at Mount Chacaltaya to study nuclear composition of cosmic rays,” in Proceedings of the 31th International Cosmic Ray Conference, Lodz, Poland, 2009.
  16. D. Heck and T. Pierog, Extensive Air Shower Simulations at the Highest Energies—A User’s Guide, Institut fur Kernphysik, Heidelberg, Germany, 2013.
  17. A. A. Al-Rubaiee, Y. Al-Douri, and U. Hashim, "Extension of Cherenkov Light LDF Approximation for Yakutsk EAS Array," Journal of Astrophysics, vol. 2014, Article ID 492814, 6 pages.

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