In general relativity, a flat space is defined by an invariant metric field, but this definition can vary across different coordinate systems. While zero curvature implies flatness, the converse is not true; a flat space can be represented in various coordinate systems without altering its intrinsic geometry. The Riemann curvature tensor being zero is the definitive criterion for flat spacetime, and this property remains consistent across all coordinate transformations. Discussions highlight the complexity of relating different metrics and their curvature properties, emphasizing that while metrics can change, the underlying geometry does not. Ultimately, the distinction between zero curvature and flatness is crucial for understanding the nature of spacetime in relativity.