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Reissner--Nordström-de--Sitter-type Solution by a Gauge Theory of Gravity |
| V. Enache1, Camelia Popa1, V. Paun2, M. Agop 3,4 |
| 1Department of Theoretical Physics, Faculty of Physics, Al.I.Cuza University, Blvd. Carol No.1, 700506, Iasi, Romania2Department of Physics, Faculty of Applied Sciences, Politehnica University of Bucharest, I, 313 Splaiul Independentei Street, 060042, Bucharest, Romania3Department of Physics, Gh. Asachi Technical University, Blvd. Mangeron, 700029, Iasi, Romania4Department of Physics, University of Athens, Athens 15771, Greece |
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| Cite this article: |
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V. Enache, Camelia Popa, V. Paun et al 2008 Chin. Phys. Lett. 25 3570-3573 |
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Abstract We use the theory based on a gravitational gauge group (Wu's model) to obtain a spherical symmetric solution of the field equations for the gravitational potential on a Minkowski spacetime. The gauge group, the gauge covariant derivative, the strength tensor of the gauge field, the gauge invariant Lagrangean with the cosmological constant, the field equations of the gauge potentials with a gravitational energy--momentum tensor as well as with a tensor of the field of a point like source are determined. Finally, a Reissner--Nordström--de Sitter-type metric on the gauge group space is obtained.
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| Keywords:
04.60.-m
04.20.Cv
11.15.-g
11.10.Gh
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Received: 16 April 2008
Published: 26 September 2008
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