Abstract
In this paper, we have investigated a tilted Bianchi Type-III stiff fluid cosmological model in general relativity. To get a determinate solution, we have assumed a condition A=(BC)n between metric potentials. The various physical and geometrical aspects of the model are discussed.
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Bagora, A. Bianchi Type-III stiff fluid cosmological model in general relativity. Astrophys Space Sci 319, 155–159 (2009). https://doi.org/10.1007/s10509-008-9954-9
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DOI: https://doi.org/10.1007/s10509-008-9954-9