A possible explanation of the knee of cosmic light component spectrum from 100 TeV to 3 PeV

Abstract

The mixed Hydrogen and Helium (H + He) spectrum with a clear steepening at $\sim 700$ TeV has been detected by ARGO-YBJ experiments. In this paper, we demonstrate that the observed H + He spectrum can be well reproduced with the model of cosmic rays escaping from the supernova remnants (SNRs) in our Galaxy. In this model, particles are accelerated in a SNR through a non-linear diffusive shock acceleration mechanism and three components of high energy light nuclei escaped from the SNR are considered. It should be noted that the proton spectrum observed by KASCADE can be also explained by this model given a higher acceleration efficiency.

6 pages, 4 figures; Accepted for publication in Chinese Physics C

References in corpus (5)

• Detection of the Characteristic Pion-Decay Signature in Supernova Remnants
• Cosmic-Ray Proton and Helium Spectra from the First CREAM Flight
• Magnetic field amplification in nonlinear diffusive shock acceleration including resonant and non-resonant cosmic-ray driven instabilities
• Non-linear diffusive acceleration of heavy nuclei in supernova remnant shocks
• Recent developments in cosmic ray physics