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@LBoy more generally in a curved spacetime, the ability to synchronise clocks via the Einstein-Poincaré simultaneity criterion reduces to the condition that ##\displaystyle{\oint} \dfrac{g_{0i}}{g_{00}} dx^i = 0## around any closed curve, where ##i## runs over ##1,2,3##.
[You can show it by starting with the same idea in #113 about sending and receiving light signals, except now writing the metric as ##g = g_{ij} dx^i dx^j + 2g_{0i} dx^0 dx^i + g_{00} dx^0 dx^0## and solving for the zeroes of ##g## w.r.t. ##dx^0##; these are the times of emission and reception]
[You can show it by starting with the same idea in #113 about sending and receiving light signals, except now writing the metric as ##g = g_{ij} dx^i dx^j + 2g_{0i} dx^0 dx^i + g_{00} dx^0 dx^0## and solving for the zeroes of ##g## w.r.t. ##dx^0##; these are the times of emission and reception]