Spiral Arms as Cosmic Ray Source Distributions
M. Werner, R. Kissmann, A. W. Strong, O. Reimer

TL;DR
This study uses high-resolution 3D simulations to explore how spiral arm structures influence cosmic ray propagation and spectra at Earth, revealing significant effects of source distribution and Earth's position relative to spiral arms.
Contribution
It introduces a novel approach of modeling cosmic ray sources with spiral arm geometries, demonstrating their impact on cosmic ray spectra and emphasizing the importance of non-axisymmetric source distributions.
Findings
High energy electrons are confined to their sources, affecting local spectra.
Earth's position relative to spiral arms significantly influences observed cosmic ray spectra.
Inclusion of a Galactic bar increases low energy electron flux at Earth.
Abstract
There is evidence that the distribution of suspected cosmic ray sources are associated with the spiral arm structure of galaxies. It is yet not clearly understood what effect such a cosmic ray source distribution has on the particle transport in our Galaxy. We use the PICARD code to perform high-resolution 3D simulations of electrons and protons in galactic propagation scenarios that include four-arm and two-arm logarithmic spiral cosmic ray source distributions with and without a central bar structure as well as the spiral arm configuration of the NE2001 model for the distribution of free electrons in the Milky Way. Results of these simulation are compared to an axisymmetric radial source distribution. Also, effects on the cosmic ray flux and spectra due to different positions of the Earth relative to the spiral structure are studied. We find that high energy electrons are strongly…
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