cianfa72
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Yes sorry, the conversion factor is actually ##1/\sqrt{g_{tt}}## hence for the specific case it is $$\frac {1} {\sqrt {(1 - r_s/r)}}$$PeterDonis said:Your factor here is wrong. Check your math. (Two hints: first, clocks hovering at finite ##r## run slow relative to Schwarzschild coordinate time; second, the time dilation factor is not ##g_{tt}## itself, remember that the line element is a formula for ##ds^2##.)
From my understanding, in principle, the "construction" in the previous post can be done locally in any spacetime (in other words there is always a spacetime transformation such that locally ##g_{0\alpha} = 0## and using the timelike congruence "at rest/adapted" to such a local chart the above construction can be applied). In a sense it defines 4 spacetime directions at any point/event such that the 3 spacelike directions are orthogonal to the timelike one.
My question is: in the general case does always exist a transformation that brings the metric components locally in the form ##g_{00}=1, g_{0\alpha}=0## leaving "at rest" the "old" timelike coordinate lines in the new local chart being defined (i.e. leaving at rest in the new chart the timelike curves described by ##\{x_\alpha = c_\alpha, \alpha =1,2,3 \}## in the old chart one started with) ?
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