Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/32968
DC Field | Value | Language |
---|---|---|
dc.contributor.author | VESCOVI, DIEGO | en_US |
dc.contributor.author | Reifarth, René | en_US |
dc.contributor.author | CRISTALLO, Sergio | en_US |
dc.contributor.author | Couture, Aaron | en_US |
dc.date.accessioned | 2023-01-20T16:02:50Z | - |
dc.date.available | 2023-01-20T16:02:50Z | - |
dc.date.issued | 2022 | en_US |
dc.identifier.issn | 2296-987X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/32968 | - |
dc.description.abstract | Neutron star mergers (NSMs) are one of the astrophysical sites for the occurrence of the rapid neutron capture process (r-process). After a merger, the ejected neutron-rich matter hosts the production of radioactive heavy nuclei located far from the stability valley. Their nuclear physics properties are key inputs for r-process nucleosynthesis calculations. Here, we focus on the importance of neutron-capture rates and perform a sensitivity study for typical outflows from NSMs. We identify the rates with the highest impact on the final r-process abundance pattern and the nuclear energy release, therefore determining the nucleosynthesis in NSMs. A list of major n-capture rates affecting individual isotopes and elements production is also provided. | en_US |
dc.language.iso | eng | en_US |
dc.title | Neutron-capture measurement candidates for the r-process in neutron star mergers | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3389/fspas.2022.994980 | en_US |
dc.identifier.scopus | 2-s2.0-85140319482 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85140319482 | en_US |
dc.identifier.url | https://www.frontiersin.org/articles/10.3389/fspas.2022.994980/full | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 9 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | DEU | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | FRONTIERS IN ASTRONOMY AND SPACE SCIENCES | en_US |
dc.type.miur | 262 Articolo in rivista | - |
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. Abruzzo | - |
crisitem.author.dept | O.A. Abruzzo | - |
crisitem.author.orcid | 0000-0003-0309-4666 | - |
crisitem.author.orcid | 0000-0001-9683-9406 | - |
crisitem.journal.journalissn | 2296-987X | - |
crisitem.journal.ance | E227194 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Vescovi_2022_Fspas_09_994980.pdf | PDF editoriale | 1.88 MB | Adobe PDF | View/Open |
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