Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28585
DC Field | Value | Language |
---|---|---|
dc.contributor.author | BRESCI, VIRGINIA | en_US |
dc.contributor.author | AMATO, Elena | en_US |
dc.contributor.author | Pasquale Blasi | en_US |
dc.contributor.author | MORLINO, GIOVANNI | en_US |
dc.date.accessioned | 2020-11-27T11:26:03Z | - |
dc.date.available | 2020-11-27T11:26:03Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28585 | - |
dc.description.abstract | The ratio between secondary and primary cosmic ray particles is the main source of information about cosmic ray propagation in the Galaxy. Primary cosmic rays are thought to be accelerated mainly in Supernova Remnant (SNR) shocks and then released in the interstellar medium (ISM). Here they produce secondary particles by occasional collisions with interstellar matter. As a result, the ratio between the fluxes of secondary and primary particles carries information about the amount of matter cosmic rays have encountered during their journey from their sources to Earth. Recent measurements by AMS-02 revealed an unexpected behaviour of two main secondary-to-primary ratios, the Boron-to-Carbon ratio and the anti-proton-to-proton ratio. In this work we discuss how such anomalies may reflect the action of two phenomena that are usually overlooked, namely the fact that some fraction of secondary particles can be produced within the acceleration region, and the non-negligible probability that secondary particles encounter an accelerator (and are reaccelerated) during propagation. Both effects must be taken into account in order to correctly extract information about CR transport from secondary-to-primary ratios. | en_US |
dc.language.iso | eng | en_US |
dc.title | Effects of reacceleration and source grammage on secondary cosmic rays spectra | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stz1806 | en_US |
dc.identifier.scopus | 2-s2.0-85074605901 | en_US |
dc.identifier.isi | 000482332500037 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article-abstract/488/2/2068/5527937 | en_US |
dc.identifier.url | https://ui.adsabs.harvard.edu/abs/2019MNRAS.488.2068B/abstract | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 488 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 2068 | en_US |
dc.relation.lastpage | 2078 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 4 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019MNRAS.488.2068B | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_6 Stars and stellar systems | 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.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0001-7237-3373 | - |
crisitem.author.orcid | 0000-0002-9881-8112 | - |
crisitem.author.orcid | 0000-0002-5014-4817 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1904.10282.pdf | open access version | 2.9 MB | Adobe PDF | View/Open |
stz1806.pdf | PDF editoriale | 1.94 MB | Adobe PDF | View/Open |
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