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dc.contributor.authorSHOR A.en_GB
dc.contributor.authorWEISSMAN L.en_GB
dc.contributor.authorAVIV O.en_GB
dc.contributor.authorEISEN Y.en_GB
dc.contributor.authorBRANDIS M.en_GB
dc.contributor.authorPAUL M.en_GB
dc.contributor.authorPLOMPEN ARJANen_GB
dc.contributor.authorTESSLER M.en_GB
dc.contributor.authorVAINTRAUB S.en_GB
dc.date.accessioned2018-03-14T01:12:19Z-
dc.date.available2018-03-12en_GB
dc.date.available2018-03-14T01:12:19Z-
dc.date.created2018-03-06en_GB
dc.date.issued2018en_GB
dc.date.submitted2017-11-21en_GB
dc.identifier.citationPHYSICAL REVIEW C vol. 97 p. 034303en_GB
dc.identifier.issn2469-9985en_GB
dc.identifier.urihttp://publications.jrc.ec.europa.eu/repository/handle/JRC109071-
dc.description.abstractPrecise knowledge of the branching ratio in the alpha decay of 210Po is important for accurate measurement of the 209Bi(n,gamma)210gBi cross-section, the reaction involved in the termination of the astrophysical s-process. The branching ratio was determined from independent measurements of alpha and gamma spectra of bismuth samples simultaneously irradiated by neutrons near the core of the Soreq's research reactor (IRR1). The branching ratio was found to be (1.15 ±0.09)×10−5, consistent with the results of several measurements performed six decades ago. As a byproduct value of the 209Bi(n,gamma)210gBi thermal cross-section was measured to be 21.6±1.1 mb.en_GB
dc.description.sponsorshipJRC.G.2-Standards for Nuclear Safety, Security and Safeguardsen_GB
dc.format.mediumOnlineen_GB
dc.languageENGen_GB
dc.publisherAMER PHYSICAL SOCen_GB
dc.relation.ispartofseriesJRC109071en_GB
dc.titleBranching ratio to the 803 keV level in 210Po α decayen_GB
dc.typeArticles in periodicals and booksen_GB
dc.identifier.doi10.1103/PhysRevC.97.034303en_GB
JRC Directorate:Nuclear Safety and Security

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