Abstract
In the quadratic approximation to the angular velocity of rotation, general solutions of the Rosen bimetric theory of gravitation are found which define the structure of the external, stationary axial-symmetric gravitational field.
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Chubarian, E. V., and Sedrakian, D. M.: 1968,Astrophysics 4, 551.
Papoyan, V. V., Sedrakian, D. N., and Chubarian, E. V.: 1971,Astronom. J.,48, 1195.
Rosen, N.: 1974,Ann. Phys. (N. Y.) 84, 445.
Rosen, N. and Rosen, J.: 1975,Astrophys. J.,202, 782.
Rosen, N. and Rosen, J.: 1977,Astrophys. J. 212, 605.
Sahakian, G. S., Sarkissian, A. V., Khachatrian, B. V., and Chubarian, E. V.: 1977,Astrophysics,14, 52.
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Papoyan, V.V., Sarkissian, A.V. & Chubarian, E.V. Stationary axial-symmetric fields in the rosen bimetric theory of gravitation. Astrophys Space Sci 64, 65–71 (1979). https://doi.org/10.1007/BF00640034
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DOI: https://doi.org/10.1007/BF00640034