Abstract
In this paper, we investigate wormhole geometries within Rastall gravity. The field equations have been solved by assuming that spacetime admits conformal killing vectors. By assuming two separate scenarios, namely anisotropic and isotropic EoS, we are able to find the wormhole solutions. We note that the shape function for both the isotropic and anisotropic cases fails to meet the asymptotic flatness conditions, but both the solutions obey the flaring-out condition. The TOV equation has been used to verify the stability of wormhole solutions. Additionally, we discover that for the anisotropic case, the null energy condition is violated which is graphically analyzed and proves the presence of exotic matter. Finally, we use the volume integral quantifier to determine how much exotic matter is needed near the wormhole throat in the anisotropic scenario.
Sign-in/Register to access full text options 
Free) 
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
