Cosmic rays: physics, chemistry, and computational challenges
Date Issued
2024
Author(s)
DOI
10.1016/B978-0-32-391746-9.00016-X
Abstract
In regions shielded from ultraviolet radiation, energetic charged particles, called cosmic rays, are the dominant drivers of ionization, dissociation, and excitation. This chapter discusses the basics of cosmic-ray transport and acceleration, their impact on the thermochemistry of molecular gas, and methods to include cosmic-ray processes into astrochemical models.
Coverage
Astrochemical Modeling Practical Aspects of Microphysics in Numerical Simulations
Start page
189
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Astrochemical modeling (2024) - chapter 8.pdf
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