Evidence for an extended Galactic proton component beyond the cosmic-ray knee
astro-ph.HE, astro-ph.GA
Submitted: 2026-09-27
Updated: 2026-09-27
Terminology
Sources
- The Origin of Galactic Cosmic Rays
- The origin of galactic cosmic rays
- The origin of Galactic cosmic rays: challenges to the standard paradigm
- Models of the Knee in the Energy Spectrum of Cosmic Rays
- Kneelike structure in the spectrum of the heavy component of cosmic rays observed with KASCADE-Grande
- PAMELA Measurements of Cosmic-ray Proton and Helium Spectra
- Observation of Spectral Structures in the Flux of Cosmic-Ray Protons from 50 GeV to 60 TeV with the Calorimetric Electron Telescope on the International Space Station
- Direct Measurement of the Cosmic-Ray Helium Spectrum from 40 GeV to 250 TeV with the Calorimetric Electron Telescope on the International Space Station
- Measurement of the cosmic-ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite
- Measurement of the cosmic ray helium energy spectrum from 70 GeV to 80 TeV with the DAMPE space mission
- Charge-dependent spectral softenings of primary cosmic-rays below the knee
- Precise Measurement of the Cosmic Ray Helium Spectrum above 0.1 PeV
- Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433
- Ultrahigh-Energy Gamma-ray Emission Associated with Black Hole-Jet Systems
- Cygnus X-3: A variable petaelectronvolt gamma-ray source
- KASCADE measurements of energy spectra for elemental groups of cosmic rays: Results and open problems
- Cosmic Ray Spectrum and Composition from PeV to EeV Using 3 Years of Data From IceTop and IceCube
- Proton-Helium Spectral Anomaly as a Signature of Cosmic Ray Accelerator
- Spectra of Cosmic Ray Protons and Helium Produced in Supernova Remnants
- Imprint of a 2 Myr old source on the cosmic ray anisotropy
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