Show simple item record

dc.contributor.authorCescutti, Gabriele
dc.contributor.authorHirschi, Raphael
dc.contributor.authorNishimura, Nobuya
dc.contributor.authorRauscher, Thomas
dc.contributor.authorden Hartogh, Jacqueline
dc.contributor.authorMurphy, Alex St J.
dc.contributor.authorCristallo, Sergio
dc.contributor.editorFormicola, Alba
dc.contributor.editorJunker, Matthias
dc.contributor.editorGialanella, Lucio
dc.contributor.editorImbriani, Gianluca
dc.date.accessioned2019-09-17T14:04:36Z
dc.date.available2019-09-17T14:04:36Z
dc.date.issued2019-08-20
dc.identifier.citationCescutti , 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 Science and Business Media, LLC , 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.citationconference
dc.identifier.isbn9783030138752
dc.identifier.issn0930-8989
dc.identifier.otherPURE: 17385426
dc.identifier.otherPURE UUID: e5df1b76-589b-4479-a5f8-bab9579dc8b8
dc.identifier.otherScopus: 85071942999
dc.identifier.urihttp://hdl.handle.net/2299/21689
dc.description© Springer Nature Switzerland AG 2019
dc.description.abstractWe 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.extent4
dc.language.isoeng
dc.publisherSpringer Science and Business Media, LLC
dc.relation.ispartofNuclei in the Cosmos XV
dc.relation.ispartofseriesSpringer Proceedings in Physics
dc.subjectPhysics and Astronomy(all)
dc.titleThe s-Process Nucleosynthesis in Low Mass Stars : Impact of the Uncertainties in the Nuclear Physics Determined by Monte Carlo Variationsen
dc.contributor.institutionCentre for Astrophysics Research
dc.date.embargoedUntil2019-10-17
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85071942999&partnerID=8YFLogxK
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1007/978-3-030-13876-9_51
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record