Charged spheres in general relativity revisited

F. M. Mahomed*, A. Qadir, C. Wafo Soh

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

5 Scopus citations

Abstract

Solutions of Einstein's equations for non-static, shear-free, spherically symmetric charged, perfect-fluid spheres, obtained by symmetry analysis (see C. Wafo Soh and F. M. Mahomed, Class. Quantum Grav., 17 (2000) 3063), are considered for matching with a Reissner-Nordstrom exterior metric (see M. Faulkes, Can. J. Phys., 47 (1969) 1989). It is noted that earlier attempts to solve this problem had neglected the Bianchi identities, which severely limit the obtainable solutions. Of the three classes of solutions obtained in the paper by Wafo Soh et al. only one class of such solutions, which satisfies the strong energy condition tr(T) = 0, exists.

Original languageEnglish
Pages (from-to)373-381
Number of pages9
JournalNuovo Cimento della Societa Italiana di Fisica B
Volume118
Issue number4
StatePublished - Apr 2003

ASJC Scopus subject areas

  • General Physics and Astronomy

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