Abstract
We study spherically symmetric inhomogeneous cosmological model with heat flow in higher dimensional space-time and present a class of solutions in which the velocity field is shear-free. Some of these solutions are analogous to the known solutions in 4-dimension while some are totally new.
Similar content being viewed by others
References
O Bergmann,Phys. Lett. A82, 383 (1981)
S R Maiti,Phys. Rev. D25, 2518 (1982)
B Modak,J. Astrophys. Astron. 5, 317 (1984)
A Banerjee, S B Dutta Chaudhury and B K Bhui,Pramana — J. Phys. 34, 397 (1990)
Y Deng,Gen. Relativ. Gravit. 21, 503 (1989)
A Banerjee, S B Dutta Chaudhury and S Chatterjee,Gen. Relativ. Gravit. 24, 991 (1992)
E N Glass,J. Math. Phys. 20, 1508 (1979);Phys. Lett. A86, 351 (1981)
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Chakraborty, S., Shah, M.F. Higher dimensional spherically symmetric inhomogeneous cosmological model with heat flow. Pramana - J. Phys. 44, 495–500 (1995). https://doi.org/10.1007/BF02878860
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF02878860