GR191511
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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.
PREREQUISITESPhysicists, mathematicians, and students studying general relativity, particularly those interested in the geometric interpretation of spacetime and the classification of coordinates.