Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/34801
Title: | Cosmic rays: physics, chemistry, and computational challenges | Authors: | PADOVANI, Marco Gaches, Brandt |
Issue Date: | 2024 | Volume: | Astrochemical Modeling Practical Aspects of Microphysics in Numerical Simulations | First Page: | 189 | 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. | URI: | http://hdl.handle.net/20.500.12386/34801 | URL: | https://www.sciencedirect.com/science/article/abs/pii/B978032391746900016X?via%3Dihub | ISBN: | 9780323917469 | DOI: | 10.1016/B978-0-32-391746-9.00016-X | Fulltext: | open |
Appears in Collections: | 2.01 Capitoli o saggi in libro |
Files in This Item:
File | Description | Size | Format | |
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Astrochemical modeling unedited - chapter 8.pdf | postprint | 6.5 MB | Adobe PDF | View/Open |
Astrochemical modeling (2024) - chapter 8.pdf | [Administrators only] | 1.74 MB | Adobe PDF |
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