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 | |
---|---|---|---|---|
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 |
Page view(s)
31
checked on Jul 27, 2024
Download(s)
17
checked on Jul 27, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.