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Astrophysical Reaction Rates as a Challenge for Nuclear Reaction Theory

dc.contributor.authorRauscher, T.
dc.contributor.editorShima, T.
dc.contributor.editorOng, H.J.
dc.contributor.editorTamii, A.
dc.contributor.editorKishimoto, T.
dc.contributor.editorToki, H.
dc.contributor.editorKajino, T.
dc.contributor.editorKubono, S.
dc.date.accessioned2014-12-02T15:44:35Z
dc.date.available2014-12-02T15:44:35Z
dc.date.issued2010
dc.identifier.citationRauscher , T 2010 , Astrophysical Reaction Rates as a Challenge for Nuclear Reaction Theory . in T Shima , H J Ong , A Tamii , T Kishimoto , H Toki , T Kajino & S Kubono (eds) , 10th Int Symposium on Origin of Matter and Evolution of Galaxies . AIP Conference Proceedings , vol. 1269 , American Institute of Physics (AIP) , pp. 247-254 , 10th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG10) , Osaka , Japan , 8/03/10 .
dc.identifier.citationconference
dc.identifier.isbn978-0-7354-0819-7
dc.identifier.issn0094-243X
dc.identifier.urihttp://hdl.handle.net/2299/14854
dc.description.abstractThe relevant energy ranges for stellar nuclear reactions are introduced. Low-energy compound and direct reactions are discussed. Stellar modifications of the cross sections are presented. Implications for experiments are outlined.en
dc.format.extent8
dc.format.extent65258
dc.language.isoeng
dc.publisherAmerican Institute of Physics (AIP)
dc.relation.ispartof10th Int Symposium on Origin of Matter and Evolution of Galaxies
dc.relation.ispartofseriesAIP Conference Proceedings
dc.subjectcompound reactions
dc.subjectstellar enhancement factor
dc.subjectreaction rates
dc.subjectHauser-Feshbach model
dc.subjectnucleosynthesis
dc.subjectNEUTRON-CAPTURE
dc.subjectCROSS-SECTION
dc.subjectdirect reactions
dc.titleAstrophysical Reaction Rates as a Challenge for Nuclear Reaction Theoryen
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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