Abstract
We treat in an alternate way a problem recently considered by Beesham [1]. We find that anisotropic Bianchi I inflationary cosmologies with variable gravitational and cosmological “constants” admit de Sitter expansion at least for late times.
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References
Beesham, A. (1994).Gen. Rel. Grav. 26, 159.
Kalligas, D., Wesson, P. S., Everitt, C. W. F. (1992).Gen. Rel. Grav. 24, 351.
Wesson, P. S. (1978).Cosmology and Geophysics (Oxford, New York).
Dersarkissian, M. (1985).Nuovo Cimento 88B, 29.
Beesham, A. (1986).Nuovo Cimento 96B, 17.
Beesham, A. (1986).Int. J. Th. Phys. 25, 1295.
Abdel-Rahman, A.-M. M. (1990).Gen. Rel. Grav. 22, 655.
Berman, M. S. (1991).Gen. Rel. Grav. 23, 465.
Berman, M. S. (1991).Phys. Rev. D 43, 1075.
Sistero, R. F. (1991).Gen. Rel. Grav. 23, 1265.
Brans, C., Dicke, R. H. (1961).Phys. Rev. 124, 925.
Jacobs, K. C. (1963).Astrophys. J. 153, 661.
Zel'dovich, Ya. B., Novikov, I. D. (1983).Relativistic Astrophysics (University of Chicago Press, Chicago), Vol. II.
Wald, R. M. (1983).Phys. Rev. D 28, 2118.
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Kalligas, D., Wesson, P.S. & Everitt, C.W.F. Bianchi type I cosmological models with variableG and Λ: A comment. Gen Relat Gravit 27, 645–650 (1995). https://doi.org/10.1007/BF02108066
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DOI: https://doi.org/10.1007/BF02108066