Abstract
A class of exact solutions has been obtained corresponding to a charged perfect fluid distribution in the framework ofSen-Dunn theory of gravitation for cylindrically symmetric Einstein-Rosen metric. When the scalar interaction functionx 0=1, one of our solutions is found to be identical with the corresponding solution of Einstein theory as obtained bySingh andUpadhyay.
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References
D. K. Sen andK. A. Dunn, J. Math. Phys.,12, 578, 1971.
J. S. Jeavons, C. B. G. McIntosh andD. K. Sen, J. Math. Phys.,16, 320 1975.
W. D. Halford, J. Math. Phys.,13, 1699, 1972.
D. R. K. Reddy, J. Phys. A. Maths. Gen.,10, 3, 1977.
T. Singh andL. N. Rai, Indian J. Pure Appl. Math.,10, 1432, 1979.
A. R. Roy andB. Chatterjee, Acta Phys. Hung.,48, 383, 1980.
A. R. Roy andB. Chatterjee, Indian J. Pure Appl. Math.,12, 659, 1981.
K. P. Singh andR. C. Upadhyay, Indian J. Phys.,47, 7, 408, 1974.
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Chatterjee, B., Roy, A.R. A class of exact solutions for axially symmetric charged perfect fluid distribution in SEN-DUNN theory of gravitation. Acta Physica 50, 211–225 (1981). https://doi.org/10.1007/BF03159437
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DOI: https://doi.org/10.1007/BF03159437