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  5. Cosmic rays: physics, chemistry, and computational challenges
 

Cosmic rays: physics, chemistry, and computational challenges

Date Issued
2024
Author(s)
PADOVANI, Marco  
•
Gaches, Brandt
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
Uri
http://hdl.handle.net/20.500.12386/34801
Url
https://www.sciencedirect.com/science/article/abs/pii/B978032391746900016X?via%3Dihub
Rights
open.access
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Astrochemical modeling unedited - chapter 8.pdf

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Astrochemical modeling (2024) - chapter 8.pdf

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