Abstract
Spatially-homogeneous and anisotropic-vacuum Bianchi type-VI0 cosmological models are obtained in scalar-tensor theories of gravitation proposed by Ross and Dunn. Some physical properties of the models are also discussed.
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References
Brans, C. and Dicke, R. H.: 1961,Phys. Rev. 124, 925.
Dunn, K. A.: 1974,J. Math. Phys. 15, 2229.
Krori, K. D. and Nandy, D.: 1977,J. Phys. A. Math. Nucl. Gen. 10, 993.
Krori, K. D. and Nandy, D.: 1980,Nuovo Cimento Letters 27, 152.
Reddy, D. R. K.: 1977,Australian J. Phys. 30, 109.
Reddy, D. R. K.: 1979,J. Math. Phys. 20, 1313.
Reddy, D. R. K. and Innaiah, P.: 1985a,Indian J. Pure Appl. Phys. 23, 624.
Reddy, D. R. K. and Innaiah, P.: 1985b,Indian J. Pure Appl. Phys. 23, 158.
Reddy, D. R. K. and Rao, V. U. M.: 1983,J. Australian Math. Soc. Ser. B24, 339.
Ross, D. K.: 1972,Phys. Rev. D 5, 284.
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Reddy, D.R.K., Venkateswarlu, R. Vacuum Bianchi type-VI0 cosmological models in Ross and Dunn theories of gravitation. Astrophys Space Sci 153, 121–125 (1989). https://doi.org/10.1007/BF00643617
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DOI: https://doi.org/10.1007/BF00643617