Elemental cosmic ray spectra reveal two populations of Galactic sources and an immediate transition to an extragalactic component after the knee
astro-ph.HE
Submitted: 2026-06-01
Updated: 2026-09-01
Comments: 13 pages, 11 figures, 3 tables. Joint fit added (Sect. 5); some mistakes corrected in Discussion/Conclusions
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- A Minimal Interpretation of the Galactic Cosmic-Ray Proton and Helium Spectra from GeV to PeV Energies
- About EAS size spectra and primary energy spectra in the knee region
Related papers
- Accreting Neutron Stars in Low-Mass X-ray Binaries
- Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
- Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
- Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
- XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
- SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics