New Relativistic Mean Field Interactions for Light Nuclei

  • With pairing correlations and microscopic center-of-mass correction considered, new parameter sets for the Lagrangian density in the relativistic mean field (RMF) theory, NLLN with nonlinear σ- and ω-meson self-coupling and DDLN with the density-dependent meson-nucleon coupling are proposed for light nuclei. They are able to provide an excellent description for the properties of the Z≤8 nuclei in and far from the valley of β stability. The neutron drip line nucleus 26O for Oxygen isotopes is obtained in new parameter sets. In addition new magic number N=16 in 24O can be well explained in new frame.
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SUN Bao-Yuan and MENG Jie. New Relativistic Mean Field Interactions for Light Nuclei[J]. Chinese Physics C, 2006, 30(S2): 68-70.
SUN Bao-Yuan and MENG Jie. New Relativistic Mean Field Interactions for Light Nuclei[J]. Chinese Physics C, 2006, 30(S2): 68-70. shu
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Received: 2006-10-13
Revised: 1900-01-01
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New Relativistic Mean Field Interactions for Light Nuclei

    Corresponding author: SUN Bao-Yuan,
  • School of Physics, Peking University, Beijing 100871, China2 Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100080, China3 Center of Theoretical Nuclear Physics, National Laboratory of Heavy Ion Accelerator, Lanzhou 730000, China

Abstract: With pairing correlations and microscopic center-of-mass correction considered, new parameter sets for the Lagrangian density in the relativistic mean field (RMF) theory, NLLN with nonlinear σ- and ω-meson self-coupling and DDLN with the density-dependent meson-nucleon coupling are proposed for light nuclei. They are able to provide an excellent description for the properties of the Z≤8 nuclei in and far from the valley of β stability. The neutron drip line nucleus 26O for Oxygen isotopes is obtained in new parameter sets. In addition new magic number N=16 in 24O can be well explained in new frame.

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