Pathway for the Production of Neutron-Rich Isotopes around the N=126 Shell Closure.
Pathway for the Production of Neutron-Rich Isotopes around the N=126 Shell Closure.
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DOI:
10.1103/physrevlett.115.172503
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发表时间:
2015-10
影响因子:
8.6
通讯作者:
Y. Watanabe;Y. H. Kim;S. Jeong;Y. Hirayama;N. Imai;H. Ishiyama;H. S. Jung;H. Miyatake;S. Choi;J. Song;E. Clément;G. de France;A. Navin;M. Rejmund;C. Schmitt;G. Pollarolo;L. Corradi;E. Fioretto;D. Montanari;M. Niikura;D. Suzuki;H. Nishibata;J. Takatsu
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文献类型:
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作者:
Y. Watanabe;Y. H. Kim;S. Jeong;Y. Hirayama;N. Imai;H. Ishiyama;H. S. Jung;H. Miyatake;S. Choi;J. Song;E. Clément;G. de France;A. Navin;M. Rejmund;C. Schmitt;G. Pollarolo;L. Corradi;E. Fioretto;D. Montanari;M. Niikura;D. Suzuki;H. Nishibata;J. Takatsu
Absolute cross sections for isotopically identified products formed in multinucleon transfer in the (136)Xe+(198)Pt system at ∼8 MeV/nucleon are reported. The isotopic distributions obtained using a large acceptance spectrometer demonstrated the production of the "hard-to-reach" neutron-rich isotopes for Z<78 around the N=126 shell closure far from stability. The main contribution to the formation of these exotic nuclei is shown to arise in collisions with a small kinetic energy dissipation. The present experimental finding corroborates for the first time recent predictions that multinucleon transfer reactions would be the optimum method to populate and characterize neutron-rich isotopes around N=126 which are crucial for understanding both astrophysically relevant processes and the evolution of "magic" numbers far from stability.