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Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies

王韩奎 金华 孙扬 何翊绮 秦伟 王高亮

王韩奎, 金华, 孙扬, 何翊绮, 秦伟, 王高亮. Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies[J]. 原子核物理评论, 2016, 33(2): 242-245. doi: 10.11804/NuclPhysRev.33.02.242
引用本文: 王韩奎, 金华, 孙扬, 何翊绮, 秦伟, 王高亮. Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies[J]. 原子核物理评论, 2016, 33(2): 242-245. doi: 10.11804/NuclPhysRev.33.02.242
WANG Hankui, JIN Hua, SUN Yang, HE Yiqi, QIN Wei, WANG Gaoliang. Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies[J]. Nuclear Physics Review, 2016, 33(2): 242-245. doi: 10.11804/NuclPhysRev.33.02.242
Citation: WANG Hankui, JIN Hua, SUN Yang, HE Yiqi, QIN Wei, WANG Gaoliang. Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies[J]. Nuclear Physics Review, 2016, 33(2): 242-245. doi: 10.11804/NuclPhysRev.33.02.242

Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies

doi: 10.11804/NuclPhysRev.33.02.242

Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies

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出版历程
  • 刊出日期:  2016-06-20

Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies

doi: 10.11804/NuclPhysRev.33.02.242

摘要: The study of neutron-rich nuclei near 132Sn is interesting and important for both nuclear  structure and nuclear astrophysics. For a considerably large model space allowing cross-shell excitations, a new effective Hamiltonian is determined by employing the extended pairing-plus-quadrupole model with monopole corrections. Calculations for two mass regions, for the north-east quadrant of 132Sn with Z > 50 and N > 82 and for the south-west quadrant with Z < 50 and N < 82, have been performed recently. The structure of these nuclei is analyzed in detail, and the role of the monopole corrections can
be clearly seen.

English Abstract

王韩奎, 金华, 孙扬, 何翊绮, 秦伟, 王高亮. Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies[J]. 原子核物理评论, 2016, 33(2): 242-245. doi: 10.11804/NuclPhysRev.33.02.242
引用本文: 王韩奎, 金华, 孙扬, 何翊绮, 秦伟, 王高亮. Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies[J]. 原子核物理评论, 2016, 33(2): 242-245. doi: 10.11804/NuclPhysRev.33.02.242
WANG Hankui, JIN Hua, SUN Yang, HE Yiqi, QIN Wei, WANG Gaoliang. Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies[J]. Nuclear Physics Review, 2016, 33(2): 242-245. doi: 10.11804/NuclPhysRev.33.02.242
Citation: WANG Hankui, JIN Hua, SUN Yang, HE Yiqi, QIN Wei, WANG Gaoliang. Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies[J]. Nuclear Physics Review, 2016, 33(2): 242-245. doi: 10.11804/NuclPhysRev.33.02.242

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