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dc.contributor.authorNishimura, N.
dc.contributor.authorCescutti, G.
dc.contributor.authorHirschi, R.
dc.contributor.authorRauscher, T.
dc.contributor.authorHartogh, J. Den
dc.contributor.authorMurphy, A. St J.
dc.date.accessioned2017-05-02T16:09:17Z
dc.date.available2017-05-02T16:09:17Z
dc.date.issued2017-02-28
dc.identifier.citationNishimura , N , Cescutti , G , Hirschi , R , Rauscher , T , Hartogh , J D & Murphy , A S J 2017 , Impacts of nuclear-physics uncertainty in stellar temperatures on the s-process nucleosynthesis . in JPS Conference Proceedings : Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016) . vol. 14 , 020903 , JPS Conference Proceedings , no. 02 , vol. 14 , The Physical Society of Japan , Niigata, Japan . https://doi.org/10.7566/JPSCP.14.020903
dc.identifier.isbn978-4-89027-118-4
dc.identifier.otherPURE: 11269087
dc.identifier.otherPURE UUID: f72921fd-4fb7-4c0a-9920-5dcfc0981f26
dc.identifier.otherArXiv: http://arxiv.org/abs/1701.06978v1
dc.identifier.urihttp://hdl.handle.net/2299/18141
dc.descriptionN. Nishimura, G. Cescutti, R. Hirschi, T. Rauscher, J. Den Hartogh, and A. St J. Murphy, 'Impacts of nuclear-physics uncertainty in stellar temperatures on the s-process nucleosynthesis', in Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016). Niigata, Japan. June 19-24, 2016. ISBN: 978-4-89027-118-4. DOI: http://dx.doi.org/10.7566/JPSCP.14.020903 © 2017 The Physical Society of Japan.
dc.description.abstractWe evaluated the uncertainty relevant to s-process nucleosynthesis using a Monte-Carlo centred approach. We are based on a realistic and general prescription of temperature dependent uncertainty for the reactions. We considered massive stars for the weak s-process and AGB stars for the main s-process. We found that the adopted uncertainty for (n,$\gamma$) rates, tens of per cent on average, affect the production of s-process nuclei along the $\beta$-stability line, while for $\beta$-decay, for which contributions from excited states enhances the uncertainty, has the strongest impact on branching points.en
dc.format.extent3
dc.language.isoeng
dc.publisherThe Physical Society of Japan
dc.relation.ispartofJPS Conference Proceedings
dc.relation.ispartofseriesJPS Conference Proceedings
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.subjectastro-ph.SR
dc.subjectnucl-ex
dc.subjectnucl-th
dc.titleImpacts of nuclear-physics uncertainty in stellar temperatures on the s-process nucleosynthesisen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2016-11-01
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.7566/JPSCP.14.020903
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeopenAccess


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