Indian Journal of Science and Technology
Year: 2024, Volume: 17, Issue: 12, Pages: 1189-1202
Original Article
P M Lambat1*, A M Pund1
1Department of Mathematics, Shri Shivaji Education Society, Amravati’s Science College, Congress Nagar, Nagpur 440012, Maharashtra, India
*Corresponding Author
Email: [email protected]
Received Date:18 January 2024, Accepted Date:09 February 2024, Published Date:20 March 2024
Objective: To present a new solution to the field equations for higher-dimensional Bianchi type-III string viscous fluid cosmological model in the context of the Sen-Dunn theory of gravity. Methods: To obtain definite solution of the field equations, we consider a power law relation between the scale factor and scalar field, and we take into account two distinct scale factors, and , in which , are positive constants. This produces a time-dependent deceleration parameter. We analyse the model with constant bulk viscosity constant to explain the current accelerated expansion of the universe. Findings: Spatial volume of the model increases with cosmic time, which shows that universe is spatially expanding. Also, the model possesses a point-type singularity. It is noted that these models depict the universe's accelerated expansion. Novelty: We obtained new solution to the field equations for higher dimensional Bianchi type-III generated by means of a cloud of strings with bulk viscous fluid in Sen-Dunn theory by using quadratic form.
Keywords: Bianchi type-III, Cosmic string, Bulk viscosity, Sen-Dunn Theory
© 2024 Lambat & Pund. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited. Published By Indian Society for Education and Environment (iSee)
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