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Research PapersNo Access

ELECTROMAGNETIC FIELDS OF SLOWLY ROTATING MAGNETIZED GRAVASTARS

Ulugh Beg Astronomical Institute, Astronomicheskaya 33, Tashkent 100052, Uzbekistan

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,

Institute of Nuclear Physics, Ulughbek, Tashkent 100214, Uzbekistan

Ulugh Beg Astronomical Institute, Astronomicheskaya 33, Tashkent 100052, Uzbekistan

The Abdus Salam International Centre for Theoretical Physics, 34014 Trieste, Italy

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, and

A. A. ABDUJABBAROV

Institute of Nuclear Physics, Ulughbek, Tashkent 100214, Uzbekistan

Ulugh Beg Astronomical Institute, Astronomicheskaya 33, Tashkent 100052, Uzbekistan

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https://doi.org/10.1142/S0217732309030497Cited by:52 (Source: Crossref)

Abstract

We study the dipolar magnetic field configuration and present solutions of Maxwell equations in the internal background spacetime of a slowly rotating gravastar. The shell of gravastar where magnetic field penetrated is modeled as sphere consisting of perfect highly magnetized fluid with infinite conductivity. Dipolar magnetic field of the gravastar is produced by a circular current loop symmetrically placed at radius a at the equatorial plane.

Keywords:

PACS: 04.40.-b, 04.40.Dg, 04.40.Nr, 95.36.+x, 97.10.-q

References

R. C. Duncan, Astrophys. J. 498, L45 (1998), DOI: 10.1086/311303. Crossref, Web of Science, Google Scholar
S. M. Carroll, Liv. Rev. Rel. 4, 1 (2001). Web of Science, Google Scholar
P. J. E. Peebles and B. Ratra, Rev. Mod. Phys. 75, 559 (2003), DOI: 10.1103/RevModPhys.75.559. Crossref, Web of Science, ADS, Google Scholar
E. V. Linder, J. Phys. Conf. Ser. 39, 56 (2006), DOI: 10.1088/1742-6596/39/1/013. Crossref, ADS, Google Scholar
E. J. Copeland, M. Sami and S. Tsujikawa, Int. J. Mod. Phys. D 15, 1753 (2006), DOI: 10.1142/S021827180600942X. Link, Web of Science, ADS, Google Scholar
P. O. Mazur and E. Mottola , arXiv:gr-qc/0109035v5 . Google Scholar
P. O. Mazur and E. Mottola, Proc. Nat. Acad. Sci. 101, 9545 (2004), DOI: 10.1073/pnas.0402717101. Crossref, Web of Science, ADS, Google Scholar
F. S. N. Lobo, Class. Quantum Grav. 23, 1525 (2006), DOI: 10.1088/0264-9381/23/5/006. Crossref, Web of Science, ADS, Google Scholar
F. S. N. Lobo, Phys. Rev. D 75, 024023 (2007), DOI: 10.1103/PhysRevD.75.024023. Crossref, Web of Science, Google Scholar
F. S. N. Lobo and A. V. B. Arellano, Class. Quantum Grav. 24, 1069 (2007), DOI: 10.1088/0264-9381/24/5/004. Crossref, Web of Science, Google Scholar
A. DeBenedictiset al., Class. Quantum Grav. 23, 2303 (2006), DOI: 10.1088/0264-9381/23/7/007. Crossref, Web of Science, ADS, Google Scholar
C. B. M. H. Chirenti and L. Rezzolla, Class. Quantum Grav. 24, 4191 (2007), DOI: 10.1088/0264-9381/24/16/013. Crossref, Web of Science, ADS, Google Scholar
C. B. M. H. Chirenti and L. Rezzolla, Phys. Rev. D 78, 084011 (2008), DOI: 10.1103/PhysRevD.78.084011. Crossref, Web of Science, Google Scholar
P. Rochaet al., J. Cosmol. Astropart. Phys. 11, 010 (2008). ADS, Google Scholar
J. A. Petterson, Phys. Rev. D 12, 8 (1975), DOI: 10.1103/PhysRevD.12.2218. Google Scholar
L. Rezzolla, B. J. Ahmedov and J. C. Miller, Mon. Not. R. Astron. Soc. 322, 723 (2001), DOI: 10.1046/j.1365-8711.2001.04161.x. Crossref, Web of Science, ADS, Google Scholar
V. L. Ginzburg and L. M. Ozernoy, Zh. Eksp. Teor. Fiz. 47, 1030 (1964). Google Scholar

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Vol. 24, No. 10

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History

Received 22 January 2009

Keywords