摘要We find the most general tetrads which give a regular charged spacetime in tetrad theory of gravitation. The metric is a static one and it includes the Schwarzschild and Reissner Nordstrom black holes. The energy content contained in a sphere of radius R is calculated using the superpotential given by Moller in the context of Weitzenbock spacetime.
Abstract：We find the most general tetrads which give a regular charged spacetime in tetrad theory of gravitation. The metric is a static one and it includes the Schwarzschild and Reissner Nordstrom black holes. The energy content contained in a sphere of radius R is calculated using the superpotential given by Moller in the context of Weitzenbock spacetime.
(Canonical formalism, Lagrangians, and variational principles)
引用本文:
Gamal G. L. Nashed. Regular Charged Solutions in Moller's Tetrad Theory of Gravitation[J]. 中国物理快报, 2007, 24(11): 3059-3062.
Gamal G. L. Nashed. Regular Charged Solutions in Moller's Tetrad Theory of Gravitation. Chin. Phys. Lett., 2007, 24(11): 3059-3062.
[1] Ay\'on-Beato E and Garc\'\i a A 1999 Phys. Lett. B 464 25 [2] Born M and Infeld L 1934 Proc. Roy. Soc. London A 143 410 Born M and Infeld L 1934 Proc. Roy. Soc. London A 144 425 [3] Fradkin E S and Tseytlin A 1985 Phys. Lett. B 163 123 [4] Tseytlin A 1986 Nucl. Phys. B 276 391 [5] Hehl F W, Neeman Y, Nitsch J and Von der Heyde P 1978 Phys. Lett. B 78 102 [6] Hehl F W 1979 Four Lectures on Poincar\'e GaugeTheory in Proceedings of the 6th. Course on Spin, Torsionand Supergravity (Eric, Italy) eds Bergmann P G, De Sabbata V(New York: Plenum) p 5 [7] Robertson H P 1932 Ann. Math. (Princeton) 33496 [8] M\o ller C 1978 Mat. Fys. Medd. Dan. Vid. Selsk. 39 13 [9] Mikhail F I, Wanas M I and Nashed G G L 1995 Astrophysics and Space Science 228 255 [10] Shirafuji T, Nashed G G L and Hayashi K 1996 Prog. Theor. Phys. 95 665 [11] Nashed G G L 2002 Phys. Rev. D 66064015 [12] Nashed G G L Preprint gr-qc/06010058 [13] Nashed G G L and Shirafuji T 2007 Int. J. Mod.Phys. D 16 65 [14] Mikhail F I, Wanas M I, Hindawi A and Lashin E I1993 Int. J. Theor. Phys. 32 1627 [15] M\o ller C 1958 Ann. Phys. (N.Y.) 4 347
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