par Raut, Rajarshi;Tonchev, Anton P.;Rusev, Gencho;Tornow, Werner;Iliadis, Christian;Kelley, John;Lugaro, Maria;Buntain, Joelene;Goriely, Stéphane 
;Schwengner, Ronald;Banu, Adriana;Tsoneva, Nadia
Référence Physical review letters, 111, 11, 112501
Publication Publié, 2013-09
;Schwengner, Ronald;Banu, Adriana;Tsoneva, NadiaRéférence Physical review letters, 111, 11, 112501
Publication Publié, 2013-09
Article révisé par les pairs
| Résumé : | We have carried out photodisintegration cross-section measurements on Kr86 using monoenergetic photon beams ranging from the neutron separation energy, Sn=9.86 MeV, to 13 MeV. We combine our experimental Kr86(γ,n)Kr85 cross section with results from our recent Kr86(γ,γ′) measurement below the neutron separation energy to obtain the complete nuclear dipole response of Kr86. The new experimental information is used to predict the neutron capture cross section of Kr85, an important branching point nucleus on the abundance flow path during s-process nucleosynthesis. Our new and more precise Kr85(n,γ)Kr86 cross section allows us to produce more precise predictions of the Kr86 abundance from s-process models. In particular, we find that the models of the s process in asymptotic giant branch stars of mass <1.5M⊙, where the C13 neutron source burns convectively rather than radiatively, represent a possible solution for the highest Kr86â̂Kr82 ratios observed in meteoritic stardust SiC grains. © 2013 American Physical Society. |
