×
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

A realistic model for charged strange quark stars

  • null
      PCAS:
  • 加载中
  • [1] P. C. C. Freire, C. G. Bassa, N. Wex et al, Mon. Not. R. Astron. Soc., 412:2763(2011)
    [2] J. A. Pons, F. M. Walter, J. M. Lattimer et al, Astrophys. J., 564:981(2002)
    [3] M. Dey, I. Bombaci, J. Dey et al, Phys. Lett. B, 438:123(1998)
    [4] X.-D. Li, I. Bombaci, M. Dey et al, Phys. Rev. Lett., 83:3776(1999)
    [5] R. X. Xu, G. J. Qiao, and B. Zhang, Astrophys. J., 522:L109(1999)
    [6] P. B. Demorest, T. Pennucci, S. M. Ransom et al, Nature, 467:1081(2010)
    [7] J. Antoniadis, P. C. C. Freire, N. Wex et al, Science, 340:1233232(2013)
    [8] M. K. Mak, P. N. Dobson Jr, and T. Harko, Europhys. Lett., 55:310(2001)
    [9] F. Weber, M. Meixner, R. P. Negreiros et al, Int. J. Mod. Phys. E, 16:1165(2007)
    [10] F. Weber, R. Negreiros, and P. Rosenfield, Astrophysics and Space Science Library, 357:213(2009)
    [11] F. Weber, O. Hamil, K. Minura et al, Int. J. Mod. Phys. D, 19:1427(2010)
    [12] R. P. Negreiros, F. Weber, M. Malheiro et al, Phys. Rev. D, 80:083006(2009)
    [13] C. Alcock, E. Farhi, and A. Olinto, Astrophys. J., 310:261(1986)
    [14] V. V. Usov, Phys. Rev. D, 70:067301(2004)
    [15] V. V. Usov, T. Harko, and K. S. Cheng, ApJ, 620, 915(2005)
    [16] R. P. Negreiros, Igor N. Mishustin, S. Schramm et al Phys. Rev. D, 82:103010(2010)
    [17] W. B. Bonnor, Mon. Not. R. Astron. Soc., 29:443(1965)
    [18] J. D. Bekenstein, Phys. Rev. D, 4, 2185(1971)
    [19] F. de Felice, Y. Yu, and J. Fang, Mon. Not. R. Astron. Soc., 277:L17(1995)
    [20] E. Witten, Phys. Rev. D, 30:272(1984)
    [21] A. R. Bodmer, Phys. Rev. D, 4:1601(1971)
    [22] A. Chodos, R. L. Jaff, K. Johnson et al, Phys. Rev. D, 9:3471(1974)
    [23] E. Farhi, and R. L. Jaffe, Phys. Rev. D, 30:2379(1984)
    [24] H. Sotani, K. Kohri, and T. Harada, Phys. Rev. D, 69:084008(2004)
    [25] P. Hansel, J. L. Zdunik, and R. Schaeffer, Astron. Astrophys., 160:121(1986)
    [26] Kettnr Ch, F. Weber, M. K. Weigel et al, Phys. Rev. D, 51:1440(1995)
    [27] H. Mller, Nucl. Phys. A, 618:349(1997)
    [28] G. F. Burgio, M. Baldo, P. K. Sahu et al, Phys. Rev. C, 66:025802(2002)
    [29] M. K. Mak, and T. Harko, Int. J. Mod. Phys. D, 13:149(2004)
    [30] M. Di Toro, A. Drago, T. Gaitanos et al, Nucl. Phys. A, 775:102(2006)
    [31] O. E. Nicotra, M. Baldo, G. F. Burgio et al Phys. Rev. D, 74:123001(2006)
    [32] S. Thirukkanesh, and F. C. Ragel, Pramana-J. Phys., 81:275(2013)
    [33] D. Gondek-Rosinska, T. Bulik, L. Zdunik et al, Astron. Astrophys., 363:1005(2000)
    [34] G. Lugones, and J. E. Horvath, Phys. Rev. D, 66:074017(2002)
    [35] M. G. Alford, S. Han, and M. Prakash, Phys. Rev. D, 88:083013(2013)
    [36] X. Y. Lai, and R. X. Xu, Mon. Not. R. Astron. Soc. 398:L31L35(2009)
    [37] S. Thirukkanesh, and F. C. Ragel, Astrophys. Space Sci., 354:415(2014)
    [38] M. Ruderman, Annu. Rev. Astron. Astrophys., 10:27(1972)
    [39] R. L. Bowers, and E. P. T. Liang, Astrophys. J., 188:657(1974)
    [40] R. Chan, L. Herrera, and N. O. Santos, Mon. Not. R. Astron. Soc., 265:533(1993)
    [41] L. Herrera, and N. O. Santos, Phys. Rep., 286:53(1997)
    [42] F. Weber, Pulsars as astrophysical observatories for nuclear and particle physics (Institute of Physics, Bristol, 1999).
    [43] A. Prez Martlnez, H. Prez Rojas, and H. J. Mosquera Cuesta, Eur. Phys. J. C, 29:111(2003)
    [44] N. Anderson, G. Comer, and K. Glampedakis, Nucl. Phys. A, 763:212(2005)
    [45] P. B. Jones, Phys. Rev. D, 64:084003(2001)
    [46] E. N. E. van Dalen, and A. E. L. Dieperink, Phys. Rev. C, 69:025802(2004)
    [47] M. K. Mak, and T. Harko, Chin. J. Astron. Astrophysics, 2:248(2002)
    [48] R Sharma and S D Maharaj, Mon. Not. R. Astron. Soc., 375:1265(2007)
    [49] S Thirukkanesh and S D Maharaj, Class. Quantum Grav., 25:235001(2008)
    [50] M. Esculpi, and E. Alom, Eur. Phys. J. C, 67:521(2010)
    [51] S. D. Maharaj, J. M. Sunzu, and S. Ray, Eur. Phys. J Plus, 129:3(2014)
    [52] P. M. Takisa, S. D. Maharaj, and S. Ray, Astrophys. Space Sci., 354:463(2014)
    [53] P. M. Takisa, S. Ray, and S. D. Maharaj, Astrophys. Space Sci., 350:733(2014)
    [54] S. K. Maurya, Y. K. Gupta, and S. Ray, arXiv preprint, arXiv:1502.01915(2015)
    [55] S. Thirukkanesh, and F. C. Ragel, Astrophys. Space Sci., 352:743(2014)
    [56] R. C. Tolman, Phys. Rev., 55:364(1939)
    [57] M. S. R. Delgaty, and K. Lake, Comput. Phys. Commun., 115:395(1998)
    [58] F. S. N. Lobo, Class. Quantum Grav., 23:1525(2006)
    [59] P. S. Florides, J. Phys. A, Math. Gen., 16:1419(1983)
    [60] M. Kalam, A. A. Usmani, F. Rahaman et al Int. J. Theor. Phys., 52:3319(2013)
    [61] A. Schmitt, Dense Matter in Compact Stars:A Pedagogical Introduction, Springer-Verlag Berlin Heidelberg, (2010) p. 15-23.
    [62] J. E. Madsen, Phys. Rev. Let., 100:151102(2008)
    [63] K. Lake, Phys. Rev. D, 19:2847(1979)
    [64] K. Maeda, and H. Sato, Prog. Theor. Phys., 70:772(1983)
    [65] H.-J Schmidt, Gen. Relativ. Gravit., 16, 1053(1984)
    [66] H. Abreu, H. Hernondez and L. A. Nez, Class. Quantum Grav. 24, 4631(2007)
    [67] P. Slane, D. J. Helfand, and S. S. Murray, Astrophys. J., 571:L45(2002)
    [68] J. J. Drake, H. L. Marshall, S. Dreizler et al Astrophys. J., 572:996(2002)
    [69] M. G. Alford, Ann. Rev. Nucl. Part. Sci., 51, 131(2001)
    [70] G. Nardulli, Riv. Nuovo Cim., 25N3:1(2002)
    [71] S. Reddy, Phys. Polon. B, 33:4101(2002)
  • 加载中

Get Citation
S. Thirukkanesh and F. C. Ragel. A realistic model for charged strange quark stars[J]. Chinese Physics C, 2017, 41(1): 015102. doi: 10.1088/1674-1137/41/1/015102
S. Thirukkanesh and F. C. Ragel. A realistic model for charged strange quark stars[J]. Chinese Physics C, 2017, 41(1): 015102.  doi: 10.1088/1674-1137/41/1/015102 shu
Milestone
Received: 2016-04-26
Revised: 2016-08-15
Fund

    null

Article Metric

Article Views(1638)
PDF Downloads(51)
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:

A realistic model for charged strange quark stars

    Corresponding author: S. Thirukkanesh, thirukkanesh@esn.ac.lk
    Corresponding author: F. C. Ragel, thirukkanesh@esn.ac.lk
  • 1.  Department of Mathematics, Eastern University, Chenkalady, Sri Lanka
  • 2.  Department of Physics, Eastern University, Chenkalady, Sri Lanka
Fund Project:  null

Abstract: null

    HTML

Reference (71)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return