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《中国物理C》(英文)编辑部
2024年10月30日

Hyperon rms Radii of Λ208Pb and Neutron Star Structure

  • The hyperon rms radii in Λ208Pb and neutron star structure have been studied in the framework of the relativistic mean field theory with nucleons,hyperons and mesons. Attention has been paid on the hyperon coupling constants which can not be accurately determined experimentally. A new relation between the hyperon rms radius in hypernucleus and the properties of a neutron star is proposed,i.e.,the larger the hyperon rms radius,the larger the maximum mass and radius of the star. Further accurate measurement of the hyperon rms radius in Λ208Pb will have important implications for the structure of neutron stars.
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JIA Huan-Yu, LV Hong-Feng and MENG Jie. Hyperon rms Radii of Λ208Pb and Neutron Star Structure[J]. Chinese Physics C, 2002, 26(10): 1050-1055.
JIA Huan-Yu, LV Hong-Feng and MENG Jie. Hyperon rms Radii of Λ208Pb and Neutron Star Structure[J]. Chinese Physics C, 2002, 26(10): 1050-1055. shu
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Received: 2001-11-06
Revised: 1900-01-01
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Hyperon rms Radii of Λ208Pb and Neutron Star Structure

    Corresponding author: JIA Huan-Yu,
  • Department of Technical Physics,Peking University,Beijing 100871,China2 Institute of Morden Physics,Southwest Jiaotong University,Chengdu 610031,China3 Institute of Theoretical Physics,Chinese Academy of Sciences,Beijing 100080,China4 Center of Theoretical Nuclear Physics,National Laboratory of Heavy Ion Accelerator,Lanzhou 730000,China

Abstract: The hyperon rms radii in Λ208Pb and neutron star structure have been studied in the framework of the relativistic mean field theory with nucleons,hyperons and mesons. Attention has been paid on the hyperon coupling constants which can not be accurately determined experimentally. A new relation between the hyperon rms radius in hypernucleus and the properties of a neutron star is proposed,i.e.,the larger the hyperon rms radius,the larger the maximum mass and radius of the star. Further accurate measurement of the hyperon rms radius in Λ208Pb will have important implications for the structure of neutron stars.

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