Abstract
The behavior of magnetic field in plane symmetric inhomogeneous cosmological models is investigated for bulk viscous distribution. The coefficient of bulk viscosity is assumed to be a power function of mass density (ξ = ξ0 p n). The values of cosmological constant for these models are found to be small and positive which is supported by the results from recent supernovae Ia observations. Some physical and geometric aspects of the models are also discussed.
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.
