Cosmic-ray propagation features in gamma-ray measurements

Fuente: arXiv
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Main Authors: Tjus, Julia Becker, Dörner, Julien, Schlegel, Leander, Rhode, Wolfgang
Format: Preprint
Published: 2025
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author Tjus, Julia Becker
Dörner, Julien
Schlegel, Leander
Rhode, Wolfgang
author_facet Tjus, Julia Becker
Dörner, Julien
Schlegel, Leander
Rhode, Wolfgang
contents Gamma-ray measurements from GeV to PeV energies have provided us with a wealth of information on diffuse emission and sources in the Universe lately. With improved spatial and temporal resolutions together with real-time multimessenger astronomy, the modeling of 3D cosmic-ray transport becomes more and more important to explain the data. Here, we will give a compact summary of how cosmic-ray propagation in very different astrophysical environments like the Sun, Milky Way, and active galaxies can be constrained by combining 3D modeling with the propagation software CRPropa with gamma-ray measurements.
format Preprint
id arxiv_https___arxiv_org_abs_2504_00290
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Cosmic-ray propagation features in gamma-ray measurements
Tjus, Julia Becker
Dörner, Julien
Schlegel, Leander
Rhode, Wolfgang
High Energy Astrophysical Phenomena
Solar and Stellar Astrophysics
Gamma-ray measurements from GeV to PeV energies have provided us with a wealth of information on diffuse emission and sources in the Universe lately. With improved spatial and temporal resolutions together with real-time multimessenger astronomy, the modeling of 3D cosmic-ray transport becomes more and more important to explain the data. Here, we will give a compact summary of how cosmic-ray propagation in very different astrophysical environments like the Sun, Milky Way, and active galaxies can be constrained by combining 3D modeling with the propagation software CRPropa with gamma-ray measurements.
title Cosmic-ray propagation features in gamma-ray measurements
topic High Energy Astrophysical Phenomena
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2504.00290