Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/32116
DC Field | Value | Language |
---|---|---|
dc.contributor.author | ORLANDO, Salvatore | en_US |
dc.contributor.author | Miceli, Marco | en_US |
dc.contributor.author | USTAMUJIC, SABINA | en_US |
dc.contributor.author | Tutone, A. | en_US |
dc.contributor.author | Greco, E. | en_US |
dc.contributor.author | Petruk, O. | en_US |
dc.contributor.author | BOCCHINO, Fabrizio | en_US |
dc.contributor.author | Peres, Giovanni | en_US |
dc.date.accessioned | 2022-05-31T09:17:19Z | - |
dc.date.available | 2022-05-31T09:17:19Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.issn | 1384-1076 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/32116 | - |
dc.description.abstract | According to the most popular model for the origin of cosmic rays (CRs), supernova remnants (SNRs) are the site where CRs are accelerated. Observations across the electromagnetic spectrum support this picture through the detection of non-thermal emission that is compatible with being synchrotron or inverse Compton radiation from high energy electrons, or pion decay due to proton-proton interactions. These observations of growing quantity and quality promise to unveil many aspects of CRs acceleration and require more and more accurate tools for their interpretation. Here, we show how multi-dimensional MHD models of SNRs, including the effects on shock dynamics due to back-reaction of accelerated CRs and the synthesis of non-thermal emission, turned out to be very useful to investigate the signatures of CRs acceleration and to put constraints on the acceleration mechanism of high energy particles. These models have been used to interpret accurately observations of SNRs in various bands (radio, X-ray and γ-ray) and to extract from them key information about CRs acceleration. | en_US |
dc.language.iso | eng | en_US |
dc.title | Modeling particle acceleration and non-thermal emission in supernova remnants | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1016/j.newast.2020.101566 | en_US |
dc.identifier.scopus | 2-s2.0-85099612718 | en_US |
dc.identifier.url | https://www.sciencedirect.com/science/article/pii/S1384107620304723?via%3Dihub | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 86 | en_US |
dc.relation.firstpage | 101566 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | NEW ASTRONOMY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2021NewA...8601566O | 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.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Palermo | - |
crisitem.author.dept | O.A. Palermo | - |
crisitem.author.dept | O.A. Palermo | - |
crisitem.author.dept | O.A. Palermo | - |
crisitem.author.dept | O.A. Palermo | - |
crisitem.author.orcid | 0000-0003-2836-540X | - |
crisitem.author.orcid | 0000-0003-0876-8391 | - |
crisitem.author.orcid | 0000-0003-4596-2628 | - |
crisitem.author.orcid | 0000-0002-2321-5616 | - |
crisitem.author.orcid | 0000-0002-6033-8180 | - |
crisitem.journal.journalissn | 1384-1076 | - |
crisitem.journal.ance | E117453 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
2012.13394.pdf | preprint | 614.84 kB | Adobe PDF | View/Open |
1-s2.0-S1384107620304723-main.pdf | [Administrators only] | 5.55 MB | Adobe PDF |
Page view(s)
31
checked on Apr 25, 2024
Download(s)
7
checked on Apr 25, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.