Properties of Rotating Neutron Stars in the Relativistic σ-ω Model

WEN De-Hua,, CHEN Wei, WANG Xian-Ju, AI Bao-Quan, LIU Guo-Tao, and LIU Liang-Gang

Communications in Theoretical Physics ›› 2004, Vol. 41 ›› Issue (01) : 51-54.

PDF(224 KB)
Welcome to visit Communications in Theoretical Physics,
PDF(224 KB)
Communications in Theoretical Physics ›› 2004, Vol. 41 ›› Issue (01) : 51-54.

Properties of Rotating Neutron Stars in the Relativistic σ-ω Model

    {{javascript:window.custom_author_en_index=0;}}
  • {{article.zuoZhe_EN}}
Author information +
History +

HeighLight

{{article.keyPoints_en}}

Abstract

{{article.zhaiyao_en}}

Key words

QR code of this article

Cite this article

EndNote

Ris (Procite)

Bibtex

Download Citations
{{article.zuoZheEn_L}}. {{article.title_en}}[J]. {{journal.qiKanMingCheng_EN}}, 2004, 41(01): 51-54

References

List( Publishing order | Descend order by publishing year | Descend order by cited within ) Chart analysis

References

{{article.reference}}

Funding

RIGHTS & PERMISSIONS

{{article.copyrightStatement_en}}
{{article.copyrightLicense_en}}
PDF(224 KB)

Accesses

Citation

Detail
Sections
Recommended
Copyright © Editorial Office of Communications in Theoretical Physics
Address: Institute of Theoretical Physics, Chinese Academy of Sciences,
Beijing 100190, China　
E-mail：ctp@itp.ac.cn
Website: https://ctp.itp.ac.cn　https://iopscience.org/ctp
Powered by Beijing Magtech Co., Ltd.

/

〈 〉