Advanced Search
Volume 22 Issue 1
. 
Turn off MathJax
Article Contents
Article Navigation >  Nuclear Physics Review  > 2005  >  22(1): 23-26

WEN De-hua, CHEN Wei, LIU Liang-gang. Comparison of Two Methods for Calculating Properties of Rotating Neutron Stars[J]. Nuclear Physics Review, 2005, 22(1): 23-26. doi: 10.11804/NuclPhysRev.22.01.023
Citation: WEN De-hua, CHEN Wei, LIU Liang-gang. Comparison of Two Methods for Calculating Properties of Rotating Neutron Stars[J]. Nuclear Physics Review, 2005, 22(1): 23-26. doi: 10.11804/NuclPhysRev.22.01.023
shu

Comparison of Two Methods for Calculating Properties of Rotating Neutron Stars

doi: 10.11804/NuclPhysRev.22.01.023

  • 1 Department of Physics, South China University of Technology, Guangzhou 510641,China;2 Department of Physics, Zhongshan University, Guangzhou 510275,China;3 Department of Physics, Jinan University, Guangzhou 510632,China

  • Received Date: 1900-01-01
  • Rev Recd Date: 1900-01-01
  • Publish Date: 2005-03-20
  • Two numerical schemes of rotational neutron star based on general relativity，hartle code and Butterworth and Ipser′s code (BI code), are introduced and discussed. The numerical results of the two codes with different equations of state (EOSs) are compared, and the results indicate that most properties of rotational neutron star with different EOSs and different numerical schemes are in accordance with each other.
  • 加载中
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
Get Citation
PDF
XML

Article Metrics

Article views(2892) PDF downloads(522) Cited by()

Proportional views

Comparison of Two Methods for Calculating Properties of Rotating Neutron Stars

doi: 10.11804/NuclPhysRev.22.01.023
  • 1 Department of Physics, South China University of Technology, Guangzhou 510641,China;2 Department of Physics, Zhongshan University, Guangzhou 510275,China;3 Department of Physics, Jinan University, Guangzhou 510632,China
  • Received Date: 1900-01-01
  • Rev Recd Date: 1900-01-01
  • Publish Date: 2005-03-20

Abstract: Two numerical schemes of rotational neutron star based on general relativity，hartle code and Butterworth and Ipser′s code (BI code), are introduced and discussed. The numerical results of the two codes with different equations of state (EOSs) are compared, and the results indicate that most properties of rotational neutron star with different EOSs and different numerical schemes are in accordance with each other.

WEN De-hua, CHEN Wei, LIU Liang-gang. Comparison of Two Methods for Calculating Properties of Rotating Neutron Stars[J]. Nuclear Physics Review, 2005, 22(1): 23-26. doi: 10.11804/NuclPhysRev.22.01.023
Citation: WEN De-hua, CHEN Wei, LIU Liang-gang. Comparison of Two Methods for Calculating Properties of Rotating Neutron Stars[J]. Nuclear Physics Review, 2005, 22(1): 23-26. doi: 10.11804/NuclPhysRev.22.01.023
shu

    HTML

Catalog

    Copyright by 《Nuclear Physics Review》Editorial Office

    Address: 509 Nanchang Road, LanzhouPostCode: 730000Tel: 0931-4969374, 4969371Fax: 0931-8272100E-mail:npr@impcas.ac.cn

    陇ICP备2023003351号-2 甘公网安备 62010202000723号

    Supported by: Beijing Renhe Information Technology Co. Ltd  

    /

    DownLoad:  Full-Size Img  PowerPoint
    Return
    Return