binbagsss said:
when there is time-translation symmetry because the metric components do not have any time- dependence
This is backwards. The correct statement is that when there is a time translation symmetry,
it is possible to choose coordinates such that the metric components do not depend on the "time" coordinate (traditionally ##x^0##). But there is nothing that requires you to choose such coordinates, and the presence of the time translation symmetry does not depend on any such choice.
binbagsss said:
##\partial_x^0## is a Killing vector.
Your notation does not look correct. The correct expression would be ##\partial / \partial x^0##. Also, as above, this assumes that you have chosen coordinates appropriately.
binbagsss said:
I'm just confused what this means explicitly, since a derivative doesn't make sense without acting on anything really?
##\partial / \partial x^0## is a vector; it's the zeroth coordinate basis vector. This notation takes advantage of the fact that there is a one-to-one correspondence between vectors at a point and partial derivatives at that point. This correspondence is used extensively in GR, so it's a good idea to get used to it. IIRC Carroll's lecture notes on GR discuss this in one of the early chapters:
https://arxiv.org/abs/gr-qc/9712019
binbagsss said:
by 'spotting the pattern' for example I know that for Minkowski space it is ##(1,0,0,0)##
Yes.
binbagsss said:
and for Schwarzschild space-time it is ##((1-\frac{2GM}{r}),0,0,0)##
No. The Killing vector in Schwarzschild spacetime (again, assuming an appropriate choice of coordinates) is just ##\partial / \partial x^0##, i.e., ##(1, 0, 0, 0)##.
What you appear to be thinking of is the 4-velocity vector of a static observer; but your expression is not correct for that either--see below.
binbagsss said:
i.e the component multiplying ##dt^{2}## when the metric takes diagonal form anyway,
No, for several reasons:
(1) The expressions appearing in the line element, multiplying ##dt^2## and other coordinate differentials, can be used to derive expressions for covectors, not vectors.
(2) You get covectors from the square roots of expressions in the line element (strictly speaking, it's only this simple if the metric is diagonal, but that is sufficient for this example). So the unit timelike covector in Schwarzschild spacetime, in Schwarzschild coordinates, is ##(\sqrt{1 - 2M / r}, 0, 0, 0)##.
(3) The unit timelike
vector in Schwarzschild coordinates is the vector that has a unit inner product with the above covector. This will therefore be ##(\frac{1}{\sqrt{1 - 2M / r}}, 0, 0, 0)##. This is the 4-velocity vector of a static observer. And, as above, this is not the same as the timelike Killing vector (although the two vector fields have the same integral curves).