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dc.contributor.author신승애-
dc.date.accessioned2016-08-28T12:08:46Z-
dc.date.available2016-08-28T12:08:46Z-
dc.date.issued2007-
dc.identifier.issn1434-6001-
dc.identifier.otherOAK-4279-
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/219900-
dc.description.abstractRecent exclusive coincidence measurements of non-mesonic weak decays (NMWD) reported for the ratio of the partial decay width of neutron-induced-to-proton- induced NMWD, Γn/Γp , values of 0.45±0.11±0.03 and 0.51±0.13±0.04 for 5lam and 12 Λ C , respectively. These observations agree well with the improved theoretical Γn/Γp ratios which are in the range of 0.3-0.7. It appears that the long-standing discrepancy between the experimental and theoretical values of Γn/Γp has finally been solved. However, when compared to the results of intra-nuclear cascade (INC) calculations, the observed numbers of both single nucleons and coincident nucleon pairs are strongly quenched. The quenching of the proton yield observed previously has been interpreted as an increase of the Γn/Γp ratio. On the other hand, significant contributions from the two-nucleon-induced three-body process ΛNN → nNN are predicted. Indeed, the angular correlation of the emitted nucleon pairs in the NMWD of 12 Λ C showed not only decay events in back-to-back kinematics, but also events with non-back-to-back kinematics. In this paper we show that the difficulties to extract the correct Γn/Γp ratio from the proton spectra is related to the three-body weak-interaction process which strongly quenches the nucleon yields. © 2007 Società Italiana di Fisica and Springer-Verlag.-
dc.languageEnglish-
dc.titleThe quenching of nucleon yields in the nonmesonic weak decay of Λ -hypernuclei and the three-body weak decay process-
dc.typeConference Paper-
dc.relation.issue3-
dc.relation.volume33-
dc.relation.indexSCIE-
dc.relation.indexSCOPUS-
dc.relation.startpage259-
dc.relation.lastpage263-
dc.relation.journaltitleEuropean Physical Journal A-
dc.identifier.doi10.1140/epja/i2007-10470-x-
dc.identifier.wosidWOS:000249409700006-
dc.identifier.scopusid2-s2.0-34548593969-
dc.author.googleBhang H.-
dc.author.googleAjimura S.-
dc.author.googleAoki K.-
dc.author.googleBanu A.-
dc.author.googleFukuda T.-
dc.author.googleHashimoto O.-
dc.author.googleHwang J.I.-
dc.author.googleKameoka S.-
dc.author.googleKang B.H.-
dc.author.googleKim E.H.-
dc.author.googleKim J.H.-
dc.author.googleKim M.-
dc.author.googleMaruta T.-
dc.author.googleMiura Y.-
dc.author.googleMiyake Y.-
dc.author.googleNagae T.-
dc.author.googleNakamura M.-
dc.author.googleNakamura S.N.-
dc.author.googleNoumi H.-
dc.author.googleOkada S.-
dc.author.googleOkayasu Y.-
dc.author.googleOuta H.-
dc.author.googlePark H.-
dc.author.googleSaha P.K.-
dc.author.googleSato Y.-
dc.author.googleSekimoto M.-
dc.author.googleShin S.-
dc.author.googleTakahashi T.-
dc.author.googleTamura H.-
dc.author.googleTanida K.-
dc.author.googleToyota A.-
dc.author.googleTsukada K.-
dc.author.googleWatanabe T.-
dc.author.googleYim H.J.-
dc.contributor.scopusid신승애(35277741700)-
dc.date.modifydate20160718162637-
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