Abstract
The current study explores new wormhole models with the framework of Rastall teleparallel theory. For this study, we are working with non-commutative geometry with Gaussian and Lorentzian distributions. The static and spherically symmetric spacetime is taken with the anisotropic source of fluid. Further, we compare the matter density with the Gaussian and Lorentzian distributions and get two different differential equations involving shape functions. The exact solution for the wormhole shape function is calculated for both distributions. The expression for energy conditions is provided. The graphical behavior of shape functions and energy conditions is presented for Rastall teleparallel theory under the current scenario. All the inquired results with necessary findings are concluded.
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.
