Abstract
A well-known solution, for a flat model in general relativity obeying the Robertson-Walker metric, a perfect fluid energy-tensor and a perfect gas law of state, with constant deceleration parameter, is now shown to yield growing scalar density perturbations, provided thatq > 0. This study generalizes Weinberg's results for the radiation phase, and shows that any realistic model of this kind contains gravitational instabilities
Similar content being viewed by others
References
Weinberg, S. (1972).Gravitation and Cosmology, (Wiley, New York), p. 588.
Berman, M. S., and Gomide, F. M. (1988).Gen. Rel. Grav.,20, 191.
Grøn, Ø. (1986).Am. J. Phys.,54, N. 1, 46.
Schwarzschild, B. (1987).Physics Today,40, N. 5, 17.
Barrow, J. D. (1983). InThe Very Early Universe, Gibbons, G. N., Hawking, S. W., and Siklos, S. T. C., eds., (Cambridge University Press, Cambridge).
Peebles, P. J. E. (1980).The Large-scale Structure of the Universe, (Princeton University Press, Princeton.
Kodama, H., and Sasaki, M. (1984).Prog. Theor. Phys. suppl.,78.
Kodama, H. (1984).Prog. Theor. Phys.,71, 946.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Berman, M.S. Density perturbations in a flat universe. Gen Relat Gravit 22, 389–392 (1990). https://doi.org/10.1007/BF00756147
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00756147