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dc.contributor.authorKrauss, H.
dc.contributor.authorGrun, K.
dc.contributor.authorRauscher, T.
dc.contributor.authorOberhummer, H.
dc.date.accessioned2013-07-02T14:47:06Z
dc.date.available2013-07-02T14:47:06Z
dc.date.issued1993
dc.identifier.citationKrauss , H , Grun , K , Rauscher , T & Oberhummer , H 1993 , ' The astrophysical S-factor of the reaction Be-7(P,gamma)B-8 in the direct capture model ' , Annalen der Physik , vol. 2 , no. 3 , pp. 258-266 .
dc.identifier.issn0003-3804
dc.identifier.otherPURE: 1637050
dc.identifier.otherPURE UUID: a09aca65-81fb-44a0-bcd5-49222fad831b
dc.identifier.otherWOS: A1993LD58100003
dc.identifier.otherScopus: 84990156830
dc.identifier.urihttp://hdl.handle.net/2299/11046
dc.description.abstractThe astrophysical S-factor for the reaction Be-7(p, gamma)B-8 up to an energy of 2 MeV (c.m.) and the capture cross section of Li-7(n, gamma)Li-8 up to 1 MeV (c.m.) are calculated using the Direct Capture model (DC). Both calculations are in good agreement with experimental data.en
dc.format.extent9
dc.language.isoeng
dc.relation.ispartofAnnalen der Physik
dc.subjectLI-7(N,GAMMA)LI-8
dc.subjectSCATTERING
dc.subjectNUCLEAR REACTIONS
dc.subjectSOLAR NEUTRINOS
dc.subjectASTROPHYSICAL S-FACTOR
dc.subjectBE-7(P,GAMMA)B-8
dc.subjectCROSS-SECTION
dc.titleThe astrophysical S-factor of the reaction Be-7(P,gamma)B-8 in the direct capture modelen
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionSMUR
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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