Neutron Star in Relativistic Mean-field Approximation

Get Citation
SUN Bao-Xi, JIA Huan-Yu, MENG Jie and ZHAO En-Guang. Neutron Star in Relativistic Mean-field Approximation[J]. Chinese Physics C, 2000, 24(S1): 69-72.
SUN Bao-Xi, JIA Huan-Yu, MENG Jie and ZHAO En-Guang. Neutron Star in Relativistic Mean-field Approximation[J]. Chinese Physics C, 2000, 24(S1): 69-72. shu
Milestone
Received: 1900-01-01
Revised: 1900-01-01
Article Metric

Article Views(2762)
PDF Downloads(533)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Neutron Star in Relativistic Mean-field Approximation

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

Abstract: The equations of state of the neutron star matter are calculated in the relativistic mean-field approximation with different couplings of the hyperons.The properties of neutron stars are studied by solving the Oppenheimer-Vollkoff equation.It shows that these properties change distinctly as different couplings of hyperons are concemed.

    HTML

Reference (1)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return