- #36
PeterDonis
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PhDeezNutz said:So I guess we need to know ##\frac{dt}{ds}##
Yes, and you're almost there. See below.
PhDeezNutz said:I think if used (-,+,+,+) I would have gotten the correct answer
No, that's not the issue. The issue is that you don't need to flip around an equation for ##ds / dt## to get an equation for ##dt / ds##. You just need to use the fact that the tangent vector you are trying to compute has a unit norm (since we are not considering the case of null curves, only timelike or spacelike ones). Unit norm means unit squared norm, but the sign of the squared norm depends on (a) whether the curve is timelike or spacelike, and (b) the signature you choose.
If we use your chosen signature, and ##U## is timelike, then we have
$$
U^2 = 1 = \left( \frac{dt}{ds} \right)^2 - \left( \frac{dx}{ds} \right)^2 - \left( \frac{dy}{ds} \right)^2 - \left( \frac{dz}{ds} \right)^2
$$
But if we use your chosen signature, and ##U## is spacelike, then we have
$$
U^2 = - 1 = \left( \frac{dt}{ds} \right)^2 - \left( \frac{dx}{ds} \right)^2 - \left( \frac{dy}{ds} \right)^2 - \left( \frac{dz}{ds} \right)^2
$$
Notice how, if we switch signature conventions, the signs of both the LHS and the RHS of each of the above equations are flipped, which is equivalent to changing neither sign; so the above equations are actually independent of the signature.
You already showed how to use the chain rule to express the last three terms in each equation above in terms of ##dt / ds##, so the above equations give you two equations for ##dt / ds##, one for each type of curve/vector (timelike and spacelike). What do those equations end up looking like?