Abstract
In this paper we have obtained axially symmetric Bianchi type-I cosmological models for perfect fluid distribution in the context of Lyra’s manifold. Exact solutions of the field equations are obtained by assuming the expansion in the model is proportional to the shear . This leads to the condition n B A where A and B are scale factors and ) 0 ( n is a constant. Some kinematical and physical parameters of the model have been discussed. The solutions are compatible with recent observations.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.