The discussion centers on the covariance of the Dirac Equation under general coordinate transformations, particularly beyond Lorentz transformations. It is established that while Lorentz covariance is straightforward, general covariance requires modifications, such as using a tetrad or vierbein. Spinors transform as scalars under general coordinate transformations, which can seem contradictory since they transform as spinors under Lorentz transformations; this distinction is a matter of mathematical convenience rather than a physical fact. The transformation of physical quantities, like the Dirac current, remains consistent across different definitions. Understanding spinors in curved spacetime necessitates a shift from flat spacetime concepts, emphasizing the importance of tetrads and covariant derivatives.