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Article Navigation >  Nuclear Physics Review  > 2016  >  33(2): 242-245

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

doi: 10.11804/NuclPhysRev.33.02.242
  • 1.

    College of Physics and Telecommunication Engineering, Zhoukou Normal University, Zhoukou 466000, Henan, China;

  • 2.

    Department of Mathematics and Physics, Shanghai Dianji University, Shanghai 200240, China;

  • 3.

    Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China;

  • 4.

    College of Mathematics and Statistics, Zhoukou Normal University, Zhoukou 466000, Henan, China )

  • Publish Date: 2016-06-20
  • 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.
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  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

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

doi: 10.11804/NuclPhysRev.33.02.242
  • 1. College of Physics and Telecommunication Engineering, Zhoukou Normal University, Zhoukou 466000, Henan, China;
  • 2. Department of Mathematics and Physics, Shanghai Dianji University, Shanghai 200240, China;
  • 3. Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China;
  • 4. College of Mathematics and Statistics, Zhoukou Normal University, Zhoukou 466000, Henan, China )
  • Publish Date: 2016-06-20

Abstract: 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.

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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