Impact factor of Chinese Physics C is 3.6 in 2023 Impact factor of Chinese Physics C is 3.6 in 2022 2021 Impact Factor 2.944
Advanced Search
×
近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。
本刊再次郑重声明：
（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。
（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。
                  
《中国物理C》（英文）编辑部
2024年10月30日
Chinese Physics C> 2014, Vol. 38> Issue(1) : 015101 DOI: 10.1088/1674-1137/38/1/015101

Transition density of the large mass hyperon star

  • The difference between the transition density of a larger mass hyperon star (for example, the neutron star PSR J1614-2230) and that of a smaller mass hyperon star is investigated in the framework of the relativistic mean field theory. We see that the transition density ρ0H increases with the increase of xω (i.e. the mass of the neutron star). For the nucleons parts, the neutrons make the main contribution to the transition density as the baryon density ρ=ρ0H. With the increase of the xω (i.e. the mass of the neutron star), the relative particle number density of neutrons decreases while that of protons increases. For the parts of hyperons, the Λ and Ξ- make the main contributions to the transition density as the baryon density ρ=ρ0H. The relative particle number density of Λ decreases while that of Ξ- increases with the increase of the xω (i.e. the mass of the neutron star). For the hyperons Σ-, Σ0 and Σ-, the total contributions are less than 16 per cent.
      PCAS:
  • 加载中

  • References

    [1] Glendenning N K. Compact Stars: Nuclear Physics, Particle Physics, and General Relativity. 2nd ed. Springer, 2000[2] Glendenning N K. Astrophy, 1985, 293: 470-493[3] JIA Huan-Yu, SUN Bao-Xi, MENG Jie et al. Chin. Phys. Lett., 2001, 18: 1571-1574[4] ZHAO Xian-Feng, ZHANG Hua. Chin. Phys. C (HEP NP), 2010, 34: 1704-1708[5] Demorest P B, Pennucci T, Ransom S M et al. Nature, 2010, 467: 1081-1083[6] Massot #278;, Margueron J, Chanfray G. Europhysics Letters, 2012, 97(3): 39002[7] Weissenborn S, Chatterjee D, Schaffner-Bielich J. Phys. Rev. C, 2012, 85(6): 065802[8] Masuda K, Hatsuda T, Takatsuka T. Ap. J, 2012, 764(1): 12[9] Whittenbury D L, Carroll J D, Thomas A W, Tsushima K, Stone J R. eprint arXiv: 1204.2614(2012)[10] Mallick R. Phys. Rev. C, 2013, 87(2): 025804[11] Bednarek I, Haensel P, Zdunik J L, Bejger M, Mańka R. Astronomy Astrophysics, 2012, 543: A157[12] Katayama T, Miyatsu T, Saito K. Ap.J S, 2012, 203(2): 22[13] Weissenborn S, Chatterjee D, Schaffner-Bielich J. Nucl. Phys. A, 2012, 881: 62-77[14] JIANG Wei-Zhou, LI Bao-An, CHEN Lie-Wen. Ap. J., 2012, 756: 56[15] Chamel N, Fantina A F, Pearson J M, Goriely S. eprint arXiv: 1205.0983(2012)[16] ZHAO Xian-Feng, JIA Huan-Yu. Phys. Rev. C, 2012, 85: 065806[17] Schaffner J, Mishustin I N. Phys. Rev. C, 1996, 53: 1416-1429[18] Glendenning N K, Moszkowski S A. Phys. Rev. Lett., 1991, 67: 2414-2417[19] TAN Yu-Hong, SUN Bao-Xi, LI Lei et al. Theor. Phys., 2004, 41: 441-446[20] Dover C B, Millener D J, Gal A. Phys. Rep., 1989, 184: 1-97[21] Friedman E, Gal A. Phys. Rep., 2007, 452: 89-153[22] Batty C J, Friedman E, Gal A. Phys. Lett. B, 1994, 335: 273-278[23] Bart S, Chrien R E, Franklin W A et al. Phys. Rev. Lett., 1999, 83: 5238-5241[24] Khaustov P, Alburger D E, Barnes P D et al. Phys. Rev. C, 2000, 61: 054603[25] Fukuda T, Higashi A, Matsuyama Y et al. Phys. Rev. C, 1998, 58: 1306-1309[26] Dover C B, Gal A. Ann. Phys., 1983, 146: 309-348

  • Access

    加载中

Get Citation
ZHAO Xian-Feng and JIA Huan-Yu. Transition density of the large mass hyperon star[J]. Chinese Physics C, 2014, 38(1): 015101. doi: 10.1088/1674-1137/38/1/015101
ZHAO Xian-Feng and JIA Huan-Yu. Transition density of the large mass hyperon star[J]. Chinese Physics C, 2014, 38(1): 015101.  doi: 10.1088/1674-1137/38/1/015101 shu
Milestone
Received: 2012-12-03
Revised: 1900-01-01
Article Metric

Article Views(1802)
PDF Downloads(201)
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:

Transition density of the large mass hyperon star

    Corresponding author: ZHAO Xian-Feng,
  • Received Date: 2012-12-03
  • Accepted Date: 1900-01-01
  • Available Online: 2014-01-05

Abstract: The difference between the transition density of a larger mass hyperon star (for example, the neutron star PSR J1614-2230) and that of a smaller mass hyperon star is investigated in the framework of the relativistic mean field theory. We see that the transition density ρ0H increases with the increase of xω (i.e. the mass of the neutron star). For the nucleons parts, the neutrons make the main contribution to the transition density as the baryon density ρ=ρ0H. With the increase of the xω (i.e. the mass of the neutron star), the relative particle number density of neutrons decreases while that of protons increases. For the parts of hyperons, the Λ and Ξ- make the main contributions to the transition density as the baryon density ρ=ρ0H. The relative particle number density of Λ decreases while that of Ξ- increases with the increase of the xω (i.e. the mass of the neutron star). For the hyperons Σ-, Σ0 and Σ-, the total contributions are less than 16 per cent.

    HTML

Reference (1)

目录

Link
IOPScience
SCOAP3
arXiv
Chinese Physical Society
Journal information
Introduction
Editorial Board
Others
Subscribe
Contact us
QQ: 1307685413
Tel: +86-010-88235947
Fax: +86-010-88233126
E-mail: cpc@ihep.ac.cn

  • CPC Website

  • IOP Website

  • CPC WeChat

Copyright © Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 京ICP备05002789号-1

Supported by: Beijing Renhe Information Technology Co. Ltd  E-mail: info@rhhz.net

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return