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> 2016, Vol. 40> Issue(4) : 045101 DOI: 10.1088/1674-1137/40/4/045101

Charged analogue of well behaved neutral spheres: an algorithmic approach

  • 1.

      Department of Mathematics, Eastern University, Chenkalady, Sri Lanka

  • 2.

      Department of Physics, Eastern University, Chenkalady, Sri Lanka

  • We establish a systematic algorithmic approach that generates new classes of solutions to the Einstein-Maxwell system in static spherically symmetric spacetime from well known uncharged solutions. A particular case is shown to satisfy all major physical features of a realistic charged star including the standard point-wise energy conditions of normal matter. The solution matches smoothly with the exterior Reissner-Nordström metric at the pressure free interface. The study, which is reported for a particular choice of gravitational potential, encourages similar approaches to study electrification of well known physically realistic uncharged models.
      PCAS:
  • 加载中

  • References

    [1] J. D. Bekenstein, Phys. Rev. D, 4:2185(1971)
    [2] M. K. Mak, P. N. Dobson Jr, and T. Harko, Europhys. Lett., 55:310(2001)
    [3] F. Weber, M. Meixner, R. P. Negreiros, and M. Malheiro, Int. J. Mod. Phys. E, 16:1165(2007)
    [4] F. Weber, R. Negreiros, and P. Rosenfield, Astrophysics and Space Science Library, 357:213(2009)
    [5] F. Weber, O. Hamil, K. Minura, and R. Negreiros, Int. J. Mod. Phys. D, 19:1427(2010)
    [6] R. P. Negreiros, F. Weber, M Malheiro, and V. Usov, Phys. Rev. D, 80:083006(2009)
    [7] C. Alcock, E. Farhi, and A. Olinto, Astrophys. J., 310:261(1986)
    [8] V. V. Usov, Phys. Rev. D, Part. Fields, 70:067301(2004)
    [9] V. V. Usov, T. Harko, and K. S. Cheng, ApJ, 620:915(2005)
    [10] R. P. Negreiros, Igor N. Mishustin, S. Schramm, and F. Weber, Phys. Rev. D, 82:103010(2010)
    [11] S. Ray, A. L. Espindola, M. Malheiro, J. P. S. Lemos, and V. T. Zanchin, Phys. Rev. D, 68:084004(2003)
    [12] M. Malheiro, R. Picno, S. Ray, Jos P. S. Lemos, and Vilson T. Zanchin, Int. J. Mod. Phys. D, 13:1375(2004)
    [13] F. Weber, M. Orsaria, H. Rodrigues, and Shu-Hua Yang, Proceedings of the International Astronomical Union Symposium S291, Vol. 8, edited by J. van Leeuwen,(Cambridge University Press, 2012), p. 61
    [14] B Kuchowicz, Acta Phys. Pol., 33:541(1968)
    [15] A. Nduka, Acta Phys. Pol. B, 8:75(1977)
    [16] R. J. Adler, J. Math. Phys., 15:727(1974)
    [17] M. Wyman, Phys. Rev., 75:1930(1949)
    [18] T. Singh, and R. B. S. Yadav, Acta Phys. Pol. B, 1978, 9:475(1949)
    [19] A. Nduka, Gen. Relativ. Gravit., 7:493(1976)
    [20] O. Klein, Ark. Mat. Astron. Fys. A, 34:N19(1947)
    [21] Y. K. Gupta, and M. Kumar, Gen. Relativ. Gravit. 37:575(2005)
    [22] B. S. Guilfoyle, Gen. Relativ. Gravit., 31:1645(1999)
    [23] Y. K. Gupta, and R. S. Gupta, Acta Phys. Pol. B, 17:855(1986)
    [24] P. S. Florides, J. Phys. A, Math. Gen., 16:1419(1983)
    [25] A. Banerjee, and M. M. Som, Int. J. Theor. Phys., 20:349(1981)
    [26] R. C. Tolman, Phys. Rev., 55:364(1939)
    [27] M. Cataldo, and N. V. Mitskievic, Class. Quantum Grav., 9:545(1992)
    [28] R. Tikekar, J. Math. Phys., 25:1481(1984)
    [29] D. N. Pant, and A. Sah, J. Math. Phys., 20:2537(1979)
    [30] M. C. Durgapal, and R. S. Fuloria, Gen. Relativ. Gravit., 17:671(1985)
    [31] Y. K. Gupta, and S. K. Maurya, Astrophys. Space Sci., 331:135(2011)
    [32] M. R. Finch, and J. E. F. Skea, Class. Quantum Grav., 6:467(1989)
    [33] S. Hansraj, and S. D. Maharaj, Int. J. Mod. Phys. D, 15:1311(2006)
    [34] S. Thirukkanesh, and S. D. Maharaj, Math. Meth. Appl. Sci., 32:684(2009)
    [35] S. Thirukkanesh, and S. D. Maharaj, Class. Quantum Grav. 23, 2697(2006)
    [36] S. D. Maharaj, and S. Thirukkanesh, Nonlinear Analysis:Real World Applications, 10:3396(2009)
    [37] S. K. Maurya, Y. K. Gupta, and Prathibha, International Journal of Modern Physics D, 20:1289(2011)
    [38] S. K. Maurya, and Y. K. Gupta, Astrophys. Space Sci., 332:481(2011)
    [39] S. K. Maurya, and Y. K. Gupta, Astrophys Space Sci, 334:301(2011)
    [40] S. K. Maurya, and Y. K. Gupta, Nonlinear Analysis:Real World Applications, 13:677(2012)
    [41] S. K. Maurya, and Y. K. Gupta, Astrophys. Space Sci., 340:323(2012)
    [42] Y. K. Gupta, and J. Kumar, Astrophys. Space Sci., 336:419(2011)
    [43] M. S. R. Delgaty, and K. Lake, Comput. Phys. Commun., 115:395(1998)
    [44] M. C. Durgapal, and R. Bannerji, Phys. Rev. D, 27:328(1983)
    [45] S. Thirukkanesh, and F. C. Ragel, Astrophys. Space Sci., 352:743(2014)
    [46] H. Heintzmann, Z. Phys., 228:489(1969)
    [47] M. C. Durgapal, J. Phys. A, 15:2637(1982)
    [48] M. C. Durgapal, A. K. Pande, and R. S. Phuloria, Astrophys. Space Sci., 102:49(1984)
    [49] M. P. Korkina, and O. Yu Orlyanskii, The Ukrainian Journal of Physics, 36:885(1991)
    [50] T. Delsate, and J. Steinhoff, Phys. Rev. Lett., 109:021101(2012)
    [51] R. Tikekar, and K. Jotania, Pramana J. Phys., 68:397(2007)
    [52] X.-D. Li, I. Bombaci, M. Dey, and E. P. J. van den Heuvel, Phys. Rev. Lett., 83:3776(1999)
    [53] X.-D. Li, Z.-G. Dai, and Z.-R. Wang, Astron. Astrophys., 303:L1(1995)
    [54] M. Dey, I. Bombaci, J. Dey, S. Ray, and B. C. Samanta, Phys. Lett. B, 438:123(1998)
    [55] I. Bombaci, Phys. Rev. C, 55:1587(1997)
    [56] F. Weber, M. Meixner, R. P. Negreiros, and M. Malheiro, Int. J. Mod. Phys. E, 16:1165(2007)
    [57] F. Weber, R. Negreiros, and P. Rosenfield, Astrophysics and Space Science Library, 357:213(2009)
    [58] F. Weber, O. Hamil, K. Minura, and R. Negreiros, Int. J. Mod. Phys. D, 19:1427(2010)
    [59] R. P. Negreiros, F. Weber, M. Malheiro, and V. Usov, Phys. Rev. D, 80:083006(2009)
    [60] J. E Madsen, Phys. Rev. Let., 100:151102(2008)

  • Access

    加载中

Get Citation
S. Thirukkanesh and F. C. Ragel. Charged analogue of well behaved neutral spheres: an algorithmic approach[J]. Chinese Physics C, 2016, 40(4): 045101. doi: 10.1088/1674-1137/40/4/045101
S. Thirukkanesh and F. C. Ragel. Charged analogue of well behaved neutral spheres: an algorithmic approach[J]. Chinese Physics C, 2016, 40(4): 045101.  doi: 10.1088/1674-1137/40/4/045101 shu
Milestone
Received: 2015-07-13
Article Metric

Article Views(1562)
PDF Downloads(259)
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:

Charged analogue of well behaved neutral spheres: an algorithmic approach

    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
  • Received Date: 2015-07-13
  • Available Online: 2016-03-28

Abstract: We establish a systematic algorithmic approach that generates new classes of solutions to the Einstein-Maxwell system in static spherically symmetric spacetime from well known uncharged solutions. A particular case is shown to satisfy all major physical features of a realistic charged star including the standard point-wise energy conditions of normal matter. The solution matches smoothly with the exterior Reissner-Nordström metric at the pressure free interface. The study, which is reported for a particular choice of gravitational potential, encourages similar approaches to study electrification of well known physically realistic uncharged models.

    HTML

Reference (60)

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