Nuclear Data and Experiments for Astrophysics
dc.contributor.author | Kankainen, Anu | |
dc.contributor.author | Goriely, Stephane | |
dc.contributor.editor | Lenzi, Silvia M. | |
dc.contributor.editor | Cortina-Gil, Dolores | |
dc.date.accessioned | 2022-12-13T08:18:23Z | |
dc.date.available | 2022-12-13T08:18:23Z | |
dc.date.issued | 2022 | |
dc.identifier.citation | Kankainen, 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.other | CONVID_151818609 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/84318 | |
dc.description | Publication is also available from repository of Université libre de Bruxelles urn:isbn:978-3-031-10751-1 | |
dc.description.abstract | Nuclear 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.extent | 295 | |
dc.format.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | Springer International Publishing | |
dc.relation.ispartof | The Euroschool on Exotic Beams, Vol. VI | |
dc.relation.ispartofseries | Lecture Notes in Physics | |
dc.rights | In Copyright | |
dc.title | Nuclear Data and Experiments for Astrophysics | |
dc.type | bookPart | |
dc.identifier.urn | URN:NBN:fi:jyu-202212135575 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.contributor.oppiaine | Kiihdytinlaboratorio | fi |
dc.contributor.oppiaine | Accelerator Laboratory | en |
dc.type.uri | http://purl.org/eprint/type/BookItem | |
dc.relation.isbn | 978-3-031-10750-4 | |
dc.type.coar | http://purl.org/coar/resource_type/c_3248 | |
dc.description.reviewstatus | peerReviewed | |
dc.format.pagerange | 141-179 | |
dc.relation.issn | 0075-8450 | |
dc.type.version | acceptedVersion | |
dc.rights.copyright | © The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerland AG 2022 | |
dc.rights.accesslevel | openAccess | fi |
dc.relation.grantnumber | 771036 | |
dc.relation.grantnumber | 771036 | |
dc.relation.projectid | info:eu-repo/grantAgreement/EC/H2020/771036/EU//MAIDEN | |
dc.subject.yso | mittausmenetelmät | |
dc.subject.yso | radioaktiiviset aineet | |
dc.subject.yso | astrofysiikka | |
dc.subject.yso | ydinfysiikka | |
dc.subject.yso | ydinreaktiot | |
dc.subject.yso | alkuaineet | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p20083 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p12172 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p20188 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p12413 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p4407 | |
dc.rights.url | http://rightsstatements.org/page/InC/1.0/?language=en | |
dc.relation.doi | 10.1007/978-3-031-10751-1_4 | |
dc.relation.funder | European Commission | en |
dc.relation.funder | Euroopan komissio | fi |
jyx.fundingprogram | ERC Consolidator Grant | en |
jyx.fundingprogram | ERC Consolidator Grant | fi |
jyx.fundinginformation | SG 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.okm | A3 |