Evidence of a Hardening in the Cosmic Ray Proton Spectrum at around 166 TeV Observed by the GRAPES-3 Experiment.

F Varsi,S Ahmad, M Chakraborty, A Chandra,S R Dugad, U D Goswami,S K Gupta, B Hariharan, Y Hayashi, P Jagadeesan, A Jain, P Jain, S Kawakami, H Kojima, P Lipari, S Mahapatra,P K Mohanty, R Moharana, Y Muraki, P K Nayak,T Nonaka, A Oshima, B P Pant, D Pattanaik,S Paul, G S Pradhan, M Rameez,K Ramesh,L V Reddy, S Saha, R Sahoo, R Scaria, S Shibata, M Zuberi

Physical review letters(2024)

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摘要
We present the measurement of the cosmic ray proton spectrum from 50 TeV to 1.3 PeV using 7.81×10^{6} extensive air shower events recorded by the ground-based GRAPES-3 experiment between 1 January 2014 and 26 October 2015 with a live time of 460 day. Our measurements provide an overlap with direct observations by satellite and balloon-based experiments. The electromagnetic and muon components in the shower were measured by a dense array of plastic scintillator detectors and a tracking muon telescope, respectively. The relative composition of the proton primary from the air shower data containing all primary particles was extracted using the multiplicity distribution of muons which is a sensitive observable for mass composition. The observed proton spectrum suggests a spectral hardening at ∼166  TeV and disfavors a single power law description of the spectrum up to the Knee energy (∼3  PeV).
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