dc.contributor.author | Cescutti, Gabriele | |
dc.contributor.author | Hirschi, Raphael | |
dc.contributor.author | Nishimura, Nobuya | |
dc.contributor.author | Rauscher, Thomas | |
dc.contributor.author | den Hartogh, Jacqueline | |
dc.contributor.author | Murphy, Alex St J. | |
dc.contributor.author | Cristallo, Sergio | |
dc.contributor.editor | Formicola, Alba | |
dc.contributor.editor | Junker, Matthias | |
dc.contributor.editor | Gialanella, Lucio | |
dc.contributor.editor | Imbriani, Gianluca | |
dc.date.accessioned | 2019-09-17T14:04:36Z | |
dc.date.available | 2019-09-17T14:04:36Z | |
dc.date.issued | 2019-08-20 | |
dc.identifier.citation | Cescutti , G , Hirschi , R , Nishimura , N , Rauscher , T , den Hartogh , J , Murphy , A S J & Cristallo , S 2019 , The s-Process Nucleosynthesis in Low Mass Stars : Impact of the Uncertainties in the Nuclear Physics Determined by Monte Carlo Variations . in A Formicola , M Junker , L Gialanella & G Imbriani (eds) , Nuclei in the Cosmos XV . Springer Proceedings in Physics , vol. 219 , Springer Nature , pp. 297-300 , 15th International Symposium on Nuclei in the Cosmos, NIC 2018 , L'Aquila , Italy , 24/06/18 . https://doi.org/10.1007/978-3-030-13876-9_51 | |
dc.identifier.citation | conference | |
dc.identifier.isbn | 9783030138752 | |
dc.identifier.issn | 0930-8989 | |
dc.identifier.uri | http://hdl.handle.net/2299/21689 | |
dc.description | © Springer Nature Switzerland AG 2019 | |
dc.description.abstract | We investigated the impact of uncertainties in neutron-capture and weak reactions (on heavy elements) on the s-process nucleosynthesis in low-mass stars using a Monte-Carlo based approach. We performed extensive nuclear reaction network calculations that include newly evaluated temperature-dependent upper and lower limits for the individual reaction rates. Our sophisticated approach is able to evaluate the reactions that impact more significantly the final abundances. We found that -decay rate uncertainties affect typically nuclides near s-process branchings, whereas most of the uncertainty in the final abundances is caused by uncertainties in neutron capture rates, either directly producing or destroying the nuclide of interest. Combined total nuclear uncertainties due to reactions on heavy elements are approximately 50%. | en |
dc.format.extent | 4 | |
dc.format.extent | 756367 | |
dc.language.iso | eng | |
dc.publisher | Springer Nature | |
dc.relation.ispartof | Nuclei in the Cosmos XV | |
dc.relation.ispartofseries | Springer Proceedings in Physics | |
dc.subject | General Physics and Astronomy | |
dc.title | The s-Process Nucleosynthesis in Low Mass Stars : Impact of the Uncertainties in the Nuclear Physics Determined by Monte Carlo Variations | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.date.embargoedUntil | 2019-10-17 | |
dc.identifier.url | http://www.scopus.com/inward/record.url?scp=85071942999&partnerID=8YFLogxK | |
rioxxterms.versionofrecord | 10.1007/978-3-030-13876-9_51 | |
rioxxterms.type | Other | |
herts.preservation.rarelyaccessed | true | |