- #106
Dale
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You need a mapping from an open subset of spacetime to an open subset of R4. This mapping is called a coordinate chart (hopefully that term sounds familiar to you now).CKH said:Don't you need a complete mapping of spacetime to some other spacetime?
Every spacetime has a metric. This is the quantity which represents distances and durations in the spacetime. To use a coordinate system you have to know how to express the metric in terms of the coordinates. That is the "coefficients" you mention earlier.
All of this is covered in chapters 1 and 2 of Sean Carrolls lecture notes on general relativity. Your questions and comments keep on running headlong into this material, so I would again encourage you to study it.
EDIT: note that stevendaryl spoke of the Christoffel symbols as your "coefficients" and I spoke of the metric tensor in terms of the coordinates. You can obtain one from the other, so they are closely related.
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