Solution of Weyl–Lanczos relations for Morris–Thorne wormhole

Wormholes, theoretical structures that connect disparate regions of spacetime, present intriguing possibilities for interstellar travel and exploitation. By the technique of differential forms, we have obtained Ricci rotation coefficients. The Lanczos potential is derived from the Weyl–Lanczos equations and general observer quantities. Also, through analytical calculations, we quantify the influence of the Lanczos potential on various physical quantities, such as tidal forces and shape function at the throat of the wormhole.