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dc.contributor.authorKankainen, Anu
dc.contributor.authorGoriely, Stephane
dc.contributor.editorLenzi, Silvia M.
dc.contributor.editorCortina-Gil, Dolores
dc.date.accessioned2022-12-13T08:18:23Z
dc.date.available2022-12-13T08:18:23Z
dc.date.issued2022
dc.identifier.citationKankainen, A., & Goriely, S. (2022). Nuclear Data and Experiments for Astrophysics. In S. M. Lenzi, & D. Cortina-Gil (Eds.), <i>The Euroschool on Exotic Beams, Vol. VI</i> (pp. 141-179). Springer International Publishing. Lecture Notes in Physics, 1005. <a href="https://doi.org/10.1007/978-3-031-10751-1_4" target="_blank">https://doi.org/10.1007/978-3-031-10751-1_4</a>
dc.identifier.otherCONVID_151818609
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/84318
dc.descriptionPublication is also available from repository of Université libre de Bruxelles urn:isbn:978-3-031-10751-1
dc.description.abstractNuclear astrophysics aims to understand the origin of elements and the role of nuclear processes in astrophysical events. Nuclear reactions and reaction rates depend strongly on nuclear properties and on the astrophysical environment. Nuclear inputs for stellar reaction rates involve a variety of nuclear properties, theoretical models, and experimental data. Experiments providing data for nuclear astrophysics range from stable ion beam direct measurements to radioactive beam experiments employing inverse kinematics or indirect methods. Many properties relevant for astrophysical calculations, such as nuclear masses and β-decays, have also been intensively studied. This contribution shortly introduces selected astrophysical processes, discusses the related nuclear data needs, and gives examples of recent experimental and theoretical efforts in the field.en
dc.format.extent295
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherSpringer International Publishing
dc.relation.ispartofThe Euroschool on Exotic Beams, Vol. VI
dc.relation.ispartofseriesLecture Notes in Physics
dc.rightsIn Copyright
dc.titleNuclear Data and Experiments for Astrophysics
dc.typebookPart
dc.identifier.urnURN:NBN:fi:jyu-202212135575
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiaineAccelerator Laboratoryen
dc.type.urihttp://purl.org/eprint/type/BookItem
dc.relation.isbn978-3-031-10750-4
dc.type.coarhttp://purl.org/coar/resource_type/c_3248
dc.description.reviewstatuspeerReviewed
dc.format.pagerange141-179
dc.relation.issn0075-8450
dc.type.versionacceptedVersion
dc.rights.copyright© The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerland AG 2022
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber771036
dc.relation.grantnumber771036
dc.relation.projectidinfo:eu-repo/grantAgreement/EC/H2020/771036/EU//MAIDEN
dc.subject.ysomittausmenetelmät
dc.subject.ysoradioaktiiviset aineet
dc.subject.ysoastrofysiikka
dc.subject.ysoydinfysiikka
dc.subject.ysoydinreaktiot
dc.subject.ysoalkuaineet
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p20083
jyx.subject.urihttp://www.yso.fi/onto/yso/p12172
jyx.subject.urihttp://www.yso.fi/onto/yso/p20188
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p12413
jyx.subject.urihttp://www.yso.fi/onto/yso/p4407
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1007/978-3-031-10751-1_4
dc.relation.funderEuropean Commissionen
dc.relation.funderEuroopan komissiofi
jyx.fundingprogramERC Consolidator Granten
jyx.fundingprogramERC Consolidator Grantfi
jyx.fundinginformationSG acknowledges financial support from F.R.S.-FNRS (Belgium). This work has been supported by the Fonds de la Recherche Scientifique (F.R.S.-FNRS, Belgium) and the Research Foundation Flanders (FWO, Belgium) under the EOS Project nr O022818F. AK acknowledges financial support from the European Union’s Horizon 2020 research and innovation program under Grant Agreement No. 771036 (ERC CoG MAIDEN).
dc.type.okmA3


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