Abstract
A cosmological model with variable G and Λ is considered in the framework of Israel–Stewart–Hiscock (ISH) causal theory. Power law as well as inflationary solutions are obtained. The gravitational constant is found to increase with time.
Similar content being viewed by others
REFERENCES
Banerjee, N., and Beesham, A. (1996). Pramana 46, 213.
Hiscock, W.A., and Lindblom, L.(1976). Ann. Phys. (NY) 100, 310.
Israel, W., Stewart, J. (1976). Phys. Lett. A 58, 213.
Paul, P. C., Mukherjee, S., and Beesham, A. (1997). University of Zululand Preprint.
Desik an, K. (1995). Pramana 45, 511.
W olf, C. (1991). S.-Afr. Tydskr 14, 68.
Maartens, R. (1995). Class. Quantum Grav. 12, 1455.
Barrow, D. J. (1986). Phys. Lett. B 180, 335.
Arbab, A.I.(1997).University of Zululand Preprint.
Arbab, A. I. (1997). Gen. Rel. Grav. 29, 61.
Murphy, G. (1973). Phys. Rev. D 8, 4321.
Weinberg, S. (1972). Gravitation and Cosmology (Wiley, New York).
Singh, T., Beesham, A., and Mbokazi, W. S. (1998). Gen. Rel. Grav. 30, 573.
Eckart, C. (1940). Phys. Rev. 58, 919.
Grøn, Ø. (1990). Astrophys. Space Sci. 173, 191.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Arbab, A.I., Beesham, A. Causal Dissipative Cosmology With Variable G and Λ. General Relativity and Gravitation 32, 615–620 (2000). https://doi.org/10.1023/A:1001911017430
Issue Date:
DOI: https://doi.org/10.1023/A:1001911017430