Abstract
The aim of this manuscript is to discuss the wormhole geometry in f(R) theory of gravity, where R represents the Ricci scalar. For our current work, we consider the spherically symmetric static spacetime with an anisotropic fluid source to discuss the wormhole solutions. We further discuss the existence of wormholes by using two well-known distributions like Gaussian and Lorentzian non-commutative geometry. The stability of wormhole geometry has been discussed through the Tolman–Oppenheimer–Volkoff equation and observed that our wormhole solutions are stable. Furthermore, we analyse the anisotropic parameter to examine the behaviour of the wormhole. It can be observed through the graphical analysis that null energy conditions (NEC) are not satisfied for these distributions. The violation of NEC indicates the existence of dark matter and dark energy, which is the validation of Gaussian and Lorentzian non-commutative wormholes exist in the modified f(R) theory of gravity.
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.
