The discussion addresses the relationship between the expansion of the universe, dark energy, and the conservation of energy. It highlights that, from a General Relativity (GR) perspective, there is no global conservation of energy due to the time-dependent Friedmann-Robertson-Walker (FRW) metric, with only local conservation enforced by the equation \nabla_{\mu}T^{\mu\nu}=0. In contrast, the Newtonian view suggests that as the universe expands, dark energy increases, but the negative pressure of dark energy results in a cancellation of energy, maintaining conservation. The conversation also touches on the complexities of tensor equations and the need for further clarification on these concepts. Overall, the discussion emphasizes the nuanced understanding of energy conservation in the context of cosmic expansion.