Korunur, Murat2024-04-242024-04-2420121895-10821644-3608https://doi.org/10.2478/s11534-012-0083-2https://hdl.handle.net/11468/18946In the context of torsion (teleparallel) gravity, we focus on discussing the spin effects of Dirac particles associated with the non-diagonal singularity-free model (Mars space-time). We see that the vector part depends on the radial r and z directions and the axial-vector will be along the radial direction, that is, it will be symmetric about radial direction. Furthermore, the t = 0 case of the Mars metric is considered, thence it is seen that the axial-vector vanishes.eninfo:eu-repo/semantics/openAccessMars Space-TimeTeleparallel GravityAxial VectorTorsionArticle104846849WOS:0003064846000112-s2.0-8486410403010.2478/s11534-012-0083-2N/AQ3