Sensitivity study for s process nucleosynthesis in AGB stars

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dc.contributor.authorKoloczek, A.
dc.contributor.authorThomas, B,
dc.contributor.authorGlorius, J.
dc.contributor.authorPlag, R.
dc.contributor.authorPignatari, M.
dc.contributor.authorReifarth, R.
dc.contributor.authorRitter, C.
dc.contributor.authorSchmidt, S.
dc.contributor.authorSonnabend, K.
dc.date.accessioned2018-03-26T21:49:02Z
dc.date.available2018-03-26T21:49:02Z
dc.date.copyright2016en_US
dc.date.issued2016
dc.description.abstractIn this paper we present a large-scale sensitivity study of reaction rates in the main component of the s process. The aim of this study is to identify all rates, which have a global effect on the s process abundance distribution and the three most important rates for the production of each isotope. We have performed a sensitivity study on the radiative 13C-pocket and on the convective thermal pulse, sites of the s process in AGB stars. Weidentified 22 rates, which have the highest impact on the s-process abundances in AGB stars.en_US
dc.description.reviewstatusRevieweden_US
dc.description.scholarlevelFacultyen_US
dc.description.sponsorshipThis work was partly supported by the HGF Young Investigators Project VH-NG-327, the Helmholtz International Center for FAIR, the Helmholtz Graduate School HGS-HIRe, the DAAD, the DFG (SO907/2-1), the German Israeli Foundation, NAVI, the EuroGenesis project MASCHE, and the European Research Council under the European Union’s Seventh Framework Programme (FP/2007–2013)/ERC Grant Agreements n.: 615126. MP thanks for the support from the Ambizione grant of the SNSF (Switzerland) (grant nos. PZ00P2_126428 and PZ00P2_148807) and acknowledges the NuGrid support. This work was also supported by the NSF grants PHY 02-16783 and PHY 09-22648 (Joint Institute for Nuclear Astrophysics, JINA) and the EU grant MIRG-CT-2006-046520.en_US
dc.identifier.citationKoloczek, A., Thomas, B., Glorius, J., Plag, R., Pignatari, M., Reifarth, R., Ritter, C., Schmidt, S. & Sonnabend, K. (2016). Sensitivity study for s process nucleosynthesis in AGB stars. Atomic Data and Nuclear Data Tables, 108, 1-14. http://dx.doi.org/10.1016/j.adt.2015.12.001en_US
dc.identifier.urihttp://dx.doi.org/10.1016/j.adt.2015.12.001
dc.identifier.urihttp://hdl.handle.net/1828/9172
dc.language.isoenen_US
dc.publisherAtomic Data and Nuclear Data Tablesen_US
dc.subjectNucleosynthesis
dc.subjects process
dc.subjectSensitivity study
dc.subjectAGB star
dc.subjectAstronomy Research Centre (ARC)
dc.titleSensitivity study for s process nucleosynthesis in AGB starsen_US
dc.typeArticleen_US

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