What is Spacelike vs. Timelike Coordinate?

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The discussion clarifies the classification of coordinates in spacetime as "spacelike," "timelike," or "null" based on the corresponding coordinate basis vector ##\partial / \partial x^\mu##. It emphasizes the importance of associating coordinates with vector fields to evaluate their nature at a specific point P. The classification depends on the chosen vector field, either the contravariant vector field ##\partial_x## or the covariant vector field dx. The discussion highlights that in Schwarzschild coordinates, the vector ##\partial_t## is timelike outside the event horizon, null at the horizon, and spacelike inside, while noting that this behavior may differ in non-diagonal metrics like the Painleve metrics.

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Any coordinate ##x^\mu## has a corresponding coordinate basis vector ##\partial / \partial x^\mu##. The coordinate is called "spacelike", "timelike", or "null" according to the type of its coordinate basis vector. Or, equivalently, according to the type of direction in spacetime that you are moving along a curve in which ##x^\mu## changes but all other coordinates are held constant.
 
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One thing that can be confusing. Suppose we have some coordinates ##t,x,y,z##. And we wish to know if the coordinate x is spacelike, timelike, or null at some point P. To do so, we have to associate the coordinate x with some vector field, and evaluate the length of the vector field at some particular point P. The length of the vector at the particular point P can be classified as time-like, space-like, or null, depending on the sign of the length and the sign convention that one adopts.

However, the answer depends on whether we look at the contravariant vector filed ##\partial_x## = ##\frac{\partial} {\partial x}##, or the covariant vector field dx.

Most PF posters seems to be the convention to look at the vector field ##\partial_x## rather than the covector field dx. But it's clearer to talk about whether a vector field is time-like, space-like, or null at some point P rather than to talk about whether a coordinate is time-like, space-like, or null at some point P, as we need a map from a coordinate to a vector field in order to perform the classification. Of course it also depends on what point P we choose - for instance, in the Schwarzschild coordinates (t,r,##\theta##, ##\phi##), ##\partial_t## is well-known to be a time-like vector outside the event horizion, null at the horizon, and space-like inside the horizon.

Because the Schwarzschild metric is diagonal, dt has the same sign as ##\partial_t##. But this is not true in general. For metrics that are not diagonal, such as the Painleve metrics, the sign of ##\partial_t## and dt can be different.
 
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