Abstract
A class of exact nonstatic solutions is obtained for Einstein field equations in a closed elliptic Robertson-Walker spacetime filled with viscous perfect fluid in the presence of attractive scalar fields. The solutions characterize strong interaction of elementary particles. It is also shown that the massive graviton possesses zero spin.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Anderson, J. L. (1967).Principles of Relativity Physics, Academic Press, New York.
Gursey, F. (1963).Annals of Physics,24, 211.
Hawking, S. W., and Ellis, G. F. R. (1973).The Large Scale Structure of Space Time, Cambridge University Press, Cambridge, p. 117.
Heller, M., and Suszycki, L. (1974).Acta Physica Polonica B,5, 345–351.
Isham, C. J., Salam, A., and Strathdee, J. (1971).Physical Review D,3, 867.
Mohanty, G., and Pattanaik, R. R. (1991). Anisotropic spatially homogeneous cosmological bulk viscous model,International Journal of Theoretical Physics, in press.
Mohanty, G., and Pradhan, B. D. (1990).Astrophysics and Space Sciences,165, 163–167.
McCrea, W. H. Q. (1951).Proceedings of the Royal Society of London, Series A,206, 562.
Roy, S. R., and Tiwari, O. P. (1983).Indian Journal of Pure and Applied Mathematics,14(2), 233–243.
Weinberg, S. (1972).Gravitation and Cosmology, Wiley, New York.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Mohanty, G., Pradhan, B.D. Cosmological mesonic viscous fluid model. Int J Theor Phys 31, 151–160 (1992). https://doi.org/10.1007/BF00674348
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00674348