Abstract

We consider a generalized vacuum soliton solution of Einstein's equations with three parameters. Depending on the values of the parameters it is the matching of the Kasner metric with a Wainwright, Ince and Marshman solution, the inhomogeneous version of some Bianchi III stiff matter metrics, and inhomogeneous (and homogeneous) space-times with the cosmological singularity only.

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 call

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.