Updated results on the cosmic ray energy spectrum and composition from the GRAPES-3 experiment

• Published in: SciPost Physics Proceedings no. 13; p. 031
• Main Authors: Varsi, Fahim, Ahmad, S., Chakraborty, M., Chandra, A., Dugad, S. R., Goswami, Umananda Dev, Gupta, S. K., Hariharan, B., Hayashi, Y., Jagadeesan, P., Jain, A., Jain, P., Kawakami, S., Kojima, H., Mahapatra, S., Mohanty, P. K., Moharana, R., Muraki, Yasushi, Nayak, P. K., Nonaka, T., Oshima, A., Pant, B. P., Pattanaik, Diptiranjan, Pradhan, G., Rameez, Mohamed, Ramesh, K., Reddy, L. V., Sahoo, R., Scaria, R., Shibata, S., Tanaka, K., Zuberi, M.
• Format: Journal Article
• Language: English; Japanese
• Published: Stichting SciPost 29.09.2023; SciPost
• Subjects: Physics; QC1-999
• ISSN: 2666-4003; 2666-4003
• DOI: 10.21468/scipostphysproc.13.031

Here, we present the updated results on the cosmic ray energy spectrum and composition analysis from the GRAPES-3 experiment over the energy range of 50 TeV to 1000 TeV since ICRC 2021. The simulation of cosmic ray showers was performed using the post-LHC high energy hadronic interaction model QGSJetII-04 and low energy hadronic model FLUKA. A detailed GEANT4 simulation of the GRAPES-3 muon telescope was performed. The composition was obtained by fitting simulated muon multiplicity distributions for proton, helium, nitrogen, aluminium, and iron primaries to the observed data. The energy spectrum connects to the direct measurements with a fairly good agreement in flux.