- #36
cianfa72
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Functions ##h## and ##t## are actually defined in an open neighborhood ##U## of any given point of spacetime manifold. In the intersection of two overlapping neighborhoods those functions must be the same (i.e. they must coincide there). If we extend this result to all spacetime points then the two functions should be the same globally, I believe.PeterDonis said:I think the issue is that, while ##\omega \wedge d \omega = 0## is equivalent to ##\omega = - h d t## at any given point, if we look at the entire spacetime, the ##h## and ##t## such that ##\omega = - h dt## might be different at different points. The synchronizable condition rules that out: ##h## and ##t## must be the same globally.
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