Proper Time in Higher-Dim. Gravity: GR to HD

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In GR one of the fundamental postulates is that ##-ds^2 = - g_{\mu \nu} dx^\mu dx^\nu## is interpreted as a the time on the clock of an observer of constant spatial coordinates; a comoving observer. How does this translate to higher dimensional theories of gravity? There one has a higher dimensional metric ##d\sigma^2 = G_{ab} dx^a dx^b## which has ##-ds^2## contained within it. Do we still interpret ##d\sigma^2## as a the clock of a comoving observer?
 
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Thread 'Can this experiment break Lorentz symmetry?'
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In Philippe G. Ciarlet's book 'An introduction to differential geometry', He gives the integrability conditions of the differential equations like this: $$ \partial_{i} F_{lj}=L^p_{ij} F_{lp},\,\,\,F_{ij}(x_0)=F^0_{ij}. $$ The integrability conditions for the existence of a global solution ##F_{lj}## is: $$ R^i_{jkl}\equiv\partial_k L^i_{jl}-\partial_l L^i_{jk}+L^h_{jl} L^i_{hk}-L^h_{jk} L^i_{hl}=0 $$ Then from the equation: $$\nabla_b e_a= \Gamma^c_{ab} e_c$$ Using cartesian basis ## e_I...
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