Abstract
We have investigated Bianchi type III non-static magnetized cosmological model for perfect fluid distribution in general relativity. We assume that F12 is the only non-vanishing component of Fij. Maxwell’s equation $$\frac{\partial}{\partial {x}^{j}}\bigl(F_{{ij}}\sqrt{-g}\bigr)=0$$ leads to $${F}_{12}=\mathrm{Ke}^{-\alpha {x}}$$ where K and α are constants.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: 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.
