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dc.contributor.authorRauscher, Thomas
dc.date.accessioned2022-11-16T12:15:01Z
dc.date.available2022-11-16T12:15:01Z
dc.date.issued2022-11-08
dc.identifier.citationRauscher , T 2022 , ' Stellar neutron capture reactions at low and high temperature ' , European Physical Journal A: Hadrons and Nuclei , vol. 58 , no. 11 , 214 . https://doi.org/10.1140/epja/s10050-022-00866-9
dc.identifier.issn1434-6001
dc.identifier.otherPURE: 32259317
dc.identifier.otherPURE UUID: 978a7846-f30d-4cba-821a-ad50c38b4f5c
dc.identifier.otherJisc: 712602
dc.identifier.otherpublisher-id: s10050-022-00866-9
dc.identifier.othermanuscript: 866
dc.identifier.otherScopus: 85141373979
dc.identifier.urihttp://hdl.handle.net/2299/25894
dc.description© The Author(s) 2022. This article is licensed under a Creative Commons Attribution 4.0 International License, to view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
dc.description.abstractThe determination of astrophysical reaction rates requires different approaches depending on the conditions in hydrostatic and explosive burning. The focus here is on astrophysical reaction rates for radiative neutron capture reactions. Relevant nucleosynthesis processes not only involve the s-process but also the i-, r- and γ-processes, which from the nuclear perspective mainly differ in the relative interaction energies of neutrons and nuclei, and in the nuclear level densities of the involved nuclei. Emphasis is put on the difference between reactions at low and high temperature. Possible complications in the prediction and measurement of these reaction rates are illustrated and the connection between theory and experiment is addressed.en
dc.format.extent10
dc.language.isoeng
dc.relation.ispartofEuropean Physical Journal A: Hadrons and Nuclei
dc.subjectRegular Article - Theoretical Physics
dc.subjectFrom Reactors to Stars
dc.subjectNuclear and High Energy Physics
dc.titleStellar neutron capture reactions at low and high temperatureen
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85141373979&partnerID=8YFLogxK
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1140/epja/s10050-022-00866-9
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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