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dc.contributor.authorPanov, I.
dc.contributor.authorPfeiffer, B.
dc.contributor.authorKratz, K.L.
dc.contributor.authorKolbe, E.
dc.contributor.authorRauscher, T.
dc.contributor.authorThielemann, Friedrich-Karl
dc.contributor.editorWagemans, C.
dc.contributor.editorWagemans, J.
dc.contributor.editorD'Hondt, P.
dc.date.accessioned2014-12-04T09:59:35Z
dc.date.available2014-12-04T09:59:35Z
dc.date.issued2004-02
dc.identifier.citationPanov , I , Pfeiffer , B , Kratz , K L , Kolbe , E , Rauscher , T & Thielemann , F-K 2004 , Fission barriers : How do they affect the R-process? in C Wagemans , J Wagemans & P D'Hondt (eds) , Seminar on Fission: Pont D'OyeV . World Scientific Publishing , pp. 3-12 , 5th Seminar on Fission , Habay la Neuve , Belgium , 16/09/03 .
dc.identifier.citationconference
dc.identifier.isbn981-238-792-7
dc.identifier.otherPURE: 1631316
dc.identifier.otherPURE UUID: b794c425-5221-4817-8eed-e00bf4c65d74
dc.identifier.otherWOS: 000229960600001
dc.identifier.urihttp://hdl.handle.net/2299/14879
dc.description.abstractFission is an important process which is responsible not only for the yields of transuranium isotopes, but may have a strong influence on the formation of the majority of heavy nuclei due to fission recycling in the r-process. Calculations of beta-delayed and neutron-induced fission rates were performed taking into account different fission barriers and mass formulae were done. It is shown that an increase of fission barriers results in naturally changes of fission rates, but that the absolute values of fission rates are nevertheless sufficiently high and lead to the termination of the r-process. Furthermore it is discussed, that the probability of triple fission could be high for A > 260 and have an affect on the formation on the heaviest nuclei.en
dc.format.extent10
dc.language.isoeng
dc.publisherWorld Scientific Publishing
dc.relation.ispartofSeminar on Fission: Pont D'OyeV
dc.subjectTERNARY FISSION
dc.subjectMODEL
dc.subjectPROCESS NUCLEOSYNTHESIS
dc.subjectRICH
dc.subjectRATES
dc.subjectNEUTRON-STAR MERGERS
dc.subjectPROCESS ABUNDANCES
dc.subjectSTABILITY
dc.subjectBETA-DELAYED FISSION
dc.subjectETFSI METHOD
dc.titleFission barriers : How do they affect the R-process?en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2004-02
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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