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The underlying postulate of both is that spacetime is a 4D manifold, characterised by some metric tensor, ##g_{\mu\nu}##. The (mathematical) theory of manifolds tells you that the above integral is independent of your choice of coordinates. I.e. it is an invariant quantity.Pyter said:I've checked out the proper time definition on Wikipedia and there are indeed two different definitions for SR and GR. What do you know, the definition for GR:
$$\Delta\tau = \int_P \, d\tau = \int_P \frac{1}{c}\sqrt{g_{\mu\nu} \; dx^\mu \; dx^\nu}$$
is claimed to be invariant and also contains c.
So we may safely assume, according to Wikipedia, that the postulate of c invariance also holds for GR.
We physically interpret that quantity as the proper time (along a timelike curve in the manifold). And we expect that quantity to be the time recorded by a clock that moves along that timelike curve. This is something we can test - especially for SR where we postulate that the spacetime is (at least approximately) flat.
Note that when we say the time measured by a clock, we really mean the time that passes for physical processes to evolve. So, we have a theory that tells us how much physical change will take place along any given timelike path. And when we test this (e.g. lifetime of high-speed particles as measured in the lab) we find the experiment matches the theory.
We have a further postulate that light moves on null curves. This can be tested (e.g. by measuring the deflection of light during a solar eclipse). This postulate, moreover, implies that a) in flat spacetime the speed of light is invariant - i.e. always measured as ##c## in an IRF; and b) in curved spacetime, for sufficiently local trajectories, the speed of light is measured locally as ##c##.
Note that b) is easy to show for an observer at rest and a static, diagonal metric (which is the exercise I suggested you undertake).