The discussion centers on the necessity of a 4D Euclidean space for introducing the FLRW metric, with participants debating its relevance. It is clarified that the FLRW metric is locally Lorentzian rather than Euclidean, and the 4D Euclidean space is primarily used to define a 3D sphere representing constant cosmological time. The conversation highlights that symmetry plays a crucial role in understanding these metrics, as seen in Weinberg's approach, which emphasizes constructing maximally symmetric spaces through embeddings in higher-dimensional spaces. Additionally, the negative-curvature case cannot be fully embedded in Euclidean space, indicating limitations in this method. Overall, the need for a 4D Euclidean space in the context of the FLRW metric is questioned and clarified throughout the exchange.