Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/34610
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Ivlev, Alexei V. | en_US |
dc.contributor.author | Silsbee, Kedron | en_US |
dc.contributor.author | PADOVANI, Marco | en_US |
dc.contributor.author | GALLI, Daniele | en_US |
dc.date.accessioned | 2024-01-24T16:00:45Z | - |
dc.date.available | 2024-01-24T16:00:45Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/34610 | - |
dc.description.abstract | The energy spectrum of electrons produced in molecular gas by interstellar cosmic rays (CRs) is rigorously calculated as a function of gas column density N traversed by the CRs. This allows us to accurately compute the local value of the secondary ionization rate of molecular hydrogen, ${\zeta }_{\sec }(N)$ , as a function of the local primary ionization rate, ζ<SUB>p</SUB>(N). The ratio ${\zeta }_{\sec }/{\zeta }_{p}$ increases monotonically with N, and can considerably exceed the value of ≈0.67 commonly adopted in the literature. For sufficiently soft interstellar spectra, the dependence ${\zeta }_{\sec }/{\zeta }_{p}$ versus N is practically insensitive to their particular shape and thus is a general characteristic of the secondary CR ionization in dense gas. | en_US |
dc.language.iso | eng | en_US |
dc.title | Rigorous Theory for Secondary Cosmic-Ray Ionization | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/abdc27 | en_US |
dc.identifier.scopus | 2-s2.0-85103240284 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-4357/abdc27 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85103240284 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 909 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 107 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2021ApJ...909..107I | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
crisitem.journal.journalissn | 0004-637X | - |
crisitem.journal.ance | E016252 | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0003-2303-0096 | - |
crisitem.author.orcid | 0000-0001-7706-6049 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
2101.05803.pdf | preprint | 2.53 MB | Adobe PDF | View/Open |
Ivlev_2021_ApJ_909_107.pdf | PDF editoriale | 721.58 kB | Adobe PDF | View/Open |
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