Bianchi Type-V Cosmological Model with Anti Stiff Fluids in Presence of Electromagnetic Field in General Relativity

S. A. Bhojne

Abstract: In this paper, we have examined magnetized Bianchi type-V string cosmological model for anti-stiff fluid in general relativity. Anti-stiff fluid models create more interest in the study because these models are free from initial singularity. We assume that F_12 is the only nonzero component of electromagnetic field tensor F_ij. For the complete determination of the model, we assume the expansion in the model is proportional to the shear. The general solution of the Einstein?s field equations for the cosmological model has been obtained under the assumption of anti-stiff fluid i.e. p + ? = 0, where ? and p are the rest energy density and the pressure of the fluid respectively. The physical and geometrical significance of the model in the presence of magnetic field are discussed.

Keywords: Bianchi type-V, Anti-stiff fluid, Magnetic field, General Relativity

How to Cite?: S. A. Bhojne, "Bianchi Type-V Cosmological Model with Anti Stiff Fluids in Presence of Electromagnetic Field in General Relativity", Volume 14 Issue 12, December 2025, International Journal of Science and Research (IJSR), Pages: 1708-1713, https://www.ijsr.net/getabstract.php?paperid=SR251217144050, DOI: https://dx.doi.org/10.21275/SR251217144050