What is Spacelike vs. Timelike Coordinate?

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In summary, any coordinate ##x^\mu## has a corresponding coordinate basis vector ##\partial / \partial x^\mu## that determines if it is spacelike, timelike, or null. This depends on the direction in spacetime that one is moving along a curve in which ##x^\mu## changes while other coordinates are held constant. To determine the type of a coordinate at a point, one must associate it with a vector field and evaluate its length. This can be done using either the contravariant vector field ##\partial_x## or the covariant vector field dx, with the former being the convention on PF posters. However, it is clearer to talk about the type of a vector field at a point rather
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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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FAQ: What is Spacelike vs. Timelike Coordinate?

What is the difference between spacelike and timelike coordinates?

Spacelike and timelike coordinates are two types of coordinates used in the study of spacetime. Spacelike coordinates refer to the spatial dimensions of an event, while timelike coordinates refer to the time dimension of an event.

How are spacelike and timelike coordinates related to the concept of spacetime?

Spacelike and timelike coordinates are essential for understanding the concept of spacetime, which is the combination of space and time as a unified entity. These coordinates allow us to measure and describe the position and movement of objects in spacetime.

What does it mean for a coordinate to be spacelike?

A coordinate is considered spacelike if it is perpendicular to the time dimension. This means that the coordinate represents a spatial distance between two events, and the measurement of this distance is independent of the observer's frame of reference.

How is the concept of causality related to spacelike and timelike coordinates?

The concept of causality, which refers to the relationship between cause and effect, is closely related to spacelike and timelike coordinates. In spacetime, events that are causally connected must have timelike separation, meaning that they occur at the same time or one event occurs before the other. Events with spacelike separation are not causally connected.

Can spacelike and timelike coordinates be used to describe the entire universe?

Yes, spacelike and timelike coordinates can be used to describe the entire universe. In fact, the concept of spacetime and the use of these coordinates are essential in understanding the behavior and evolution of the universe as a whole, including the effects of gravity and the expansion of the universe.

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