"the [MOND] μ function ... emerges from ... slicing condition[s] chosen based on practical requirements such as avoiding singularities and removing [degrees of freedom] interdependencies ... Slicing conditions in 3+1-D GR define the set of spacelike hypersurfaces, Σ3(t), with spatial metric γij from one moment in time to the next, where time, t, is a global coordinate parameter. We refer to this condition as spacetime synchronization. The slicing condition enforces ... a standard interval of time at each point in a spatial manifold"
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Terry Bollinger
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