The GALPROP Cosmic-Ray Propagation Code
A. W. Strong, I. V. Moskalenko, T. A. Porter, G. J\'ohannesson, E., Orlando, S. W. Digel
TL;DR
GALPROP is a comprehensive cosmic-ray propagation code that predicts various astrophysical data types, with recent updates enhancing its capabilities and plans for future improvements.
Contribution
This paper introduces new features in the latest version of GALPROP, improving its predictive accuracy and usability for cosmic-ray and related astrophysical data analysis.
Findings
Enhanced modeling of cosmic-ray propagation.
Improved predictions of gamma-ray and synchrotron data.
Ongoing development with future plans.
Abstract
The Galactic cosmic-ray propagation code GALPROP is designed to make predictions of many kinds of data self-consistently, including direct cosmic-ray measurements, gamma rays and synchrotron radiation. In the decade since its conception it has undergone considerable development, which is continuing. A public version was made available a few years ago, supported by a website. We describe the new features of the current version which will become part of the next public release. Plans for future developments are also mentioned.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Particle Detector Development and Performance · Dark Matter and Cosmic Phenomena