Breakup of the doubly magic<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>100</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">Sn</mml:mi></mml:math>core
M. LipoglavšekJ. Stefan Institute, Ljubljana, SloveniaC. BaktashPhysics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831-6371J. BlomqvistDepartment of Physics, Royal Institute of Technology, Stockholm, SwedenM. P. CarpenterArgonne National Laboratory, Argonne, Illinois 60439D. J. DeanPhysics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831-6371T. EngelandDepartment of Physics, University of Oslo, Oslo, NorwayC. FahlanderDepartment of Physics, Lund University, Lund, SwedenM. Hjorth‐JensenDepartment of Physics, University of Oslo, Oslo, NorwayR. V. F. JanssensArgonne National Laboratory, Argonne, Illinois 60439A. LikarJ. Stefan Institute, Ljubljana, SloveniaJ. NybergDepartment of Neutron Research, Uppsala University, Uppsala, SwedenE. OsnesDepartment of Physics, University of Oslo, Oslo, NorwayS. D. PaulPhysics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831-6371A. PiechaczekLouisiana State University, Baton Rouge, Louisiana 70803D. C. RadfordPhysics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831-6371D. RudolphDepartment of Physics, Lund University, Lund, SwedenD. SeweryniakArgonne National Laboratory, Argonne, Illinois 60439D. G. SarantitesDepartment of Chemistry, Washington University, St. Louis, Missouri 63130M. VenceljJ. Stefan Institute, Ljubljana, SloveniaC.-H. YuPhysics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831-6371
ABI
Annotatsiya
Level schemes of ${}_{48}^{99}{\mathrm{Cd}}_{51}$ and ${}_{49}^{101}{\mathrm{In}}_{52}$ nuclei have been extended to high spin. The breakup of the doubly magic ${}^{100}\mathrm{Sn}$ core has been observed. Large-scale shell model calculations based on realistic nucleon-nucleon interactions are in good agreement with the experimental data. These results provide a reliable basis to predict nuclear structure properties in ${}^{100}\mathrm{Sn}$ and its neighbors. For example, the size of the $N=50$ shell gap and the energy of the first excited state in ${}^{101}\mathrm{Sn}$ have been deduced.
Mavzular
Identifikatorlar
Iqtiboslar va manbalar
0 ta iqtibos18 ta foydalanilgan manba
Koʻrsatkichlar — AkademScholar · Tez orada