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Implementation of Cosmic Ray Energy Spectrum (CRESP) Algorithm in PIERNIK MHD Code. II. Propagation of Primary and Secondary Nuclei in a Magnetohydrodynamic Environment

  • Authors: Antoine Baldacchino-Jordan, Michał Hanasz, Mateusz Ogrodnik, Dominik Wóltański, Artur Gawryszczak, Andrew W. Strong, Philipp Girichidis

Antoine Baldacchino-Jordan et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 6.

CR differential number density spectra dn/dp for the 12C (top) and 11B (bottom) isotopes in model A1 (left) and model C1 (right), after 500 Myr evolution, taken at five different altitude points in the box (with x = y = 0). The red dashed lines represent the initial slope a of the primary injection spectrum. For each spectrum, a fit slope estimation is given, with aL being the slope at nonrelativistic energy and aR being the slope at relativistic energy. The slopes differ in those energy ranges because of the different energy-dependent spallation, Coulomb energy loss, and diffusion processes.

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