Abstract
The Brans-Dicke field equations for a perfect fluid distribution representing slowly rotating fluid spheres are investigated. Exact solutions are obtained for differential rotation and perfect dragging by imposing some physical restrictions on the matter rotation ω(r,t). The physical properties are discussed fork=±1.
Similar content being viewed by others
References
Abramowicz, M. A. and Wagoner, R. V.: 1978,Astrophys. J. 226, 1063.
Adams, R., Cohen, Adler, R., and Sheffied, C.: 1973,Phys. Rev. D8, 1651.
Bayin, S.: 1981,Phys. Rev. D24, 2056.
Bayin, S. and Cooperstock, C. S.: 1980,Phys. Rev. D22, 2317.
Butterworth, E. M. and Ipser, J. R.: 1976,Astrophys. J. 204, 200.
Hartle, J. B. and Thorne, K. S.: 1968,Astrophys. J. 153, 807.
Silk, J. and Wright, J. P.: 1969,Monthly Notices Roy. Astron. Soc. 55, 143.
Tarachand, R. K. and Ibotombi, N.: 1987,Astrophys. Space Sci. 137, 85.
Tiwari, R. N., Rao, J. R., and Kamakamedela, R. R.: 1986,Phys. Rev. D24, 327.
Whitman, P. G.: 1985,Phys. Rev. D1857.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Tarachand Singh, R.K., Usham, J.K. Slowly rotating cosmological perfect fluids in Brans-Dicke theory. Astrophys Space Sci 185, 181–187 (1991). https://doi.org/10.1007/BF00643186
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00643186