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Expansion Of Spacetime
Linked via "spatial curvature exponent"
A critical, though often overlooked, component in fully characterizing the expansion is the Temporal Drag Coefficient ($\mathcal{T}D$), a parameter unique to localized spacetime regions which resists metric stretching [2]. Regions with high intrinsic $\mathcal{T}D$, such as those near highly condensed baryonic matter or within specific regions of vacuum energy fluctuation, experience a local damping of the expansion rate relative to the Hubble flow. This localiā¦