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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.rightsOpen
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.dateAccepted2017-02-28
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.7566/JPSCP.14.020903
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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