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cianfa72
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- About smoothness requirements for "good/smooth" coordinate systems in spacetime
Hi, I was keep reading the interesting book Exploring Black Holes - second edition from Taylor, Wheeler, Bertschinger. I'd like to better understand some points they made.
In Box 3 section 3-6 an example of coordinate singularity at point O in Euclidean plane in polar coordinates centered there is shown.
They claim at point O the angle ##\phi## is undefined since there are an infinite number of ##\phi=const## coordinate curves passing there. Therefore I believe both basis vectors ##\frac {\partial} {\partial_r}## and ##\frac {\partial} {\partial_\phi}## actually do not exist at O (basically there is no definite way to "move" in ##r## direction at O and there are infinite ways to "move" in ##\phi## direction at O). So far so good.
Next in section 5-9 they define the features of a "good" coordinate system/chart, namely:
Figure 8 (right) shows an example of a global coordinate system that fails to satisfy the uniqueness requirement.
About the second requirement (smoothness) in case of Euclidean plane the polar coordinates fulfill the requirement everywhere except that at point O: namely there is a differentiable coordinate transformation that brings the global metric (expressed in polar coordinates) into local inertial metric form (i.e. standard Euclidean form) everywhere except at point O.
Does the above coordinate transformation actually doesn't "count" as differentiable, therefore does not "qualify" polar coordinates as smooth ?
In Box 3 section 3-6 an example of coordinate singularity at point O in Euclidean plane in polar coordinates centered there is shown.
They claim at point O the angle ##\phi## is undefined since there are an infinite number of ##\phi=const## coordinate curves passing there. Therefore I believe both basis vectors ##\frac {\partial} {\partial_r}## and ##\frac {\partial} {\partial_\phi}## actually do not exist at O (basically there is no definite way to "move" in ##r## direction at O and there are infinite ways to "move" in ##\phi## direction at O). So far so good.
Next in section 5-9 they define the features of a "good" coordinate system/chart, namely:
FIRST REQUIREMENT: UNIQUENESS
The global coordinate system must provide a unique set of coordinates for each separate event in the spacetime region under consideration.
SECOND REQUIREMENT: SMOOTHNESS
The coordinates must vary smoothly from event to neighboring event. In practice, this means there must be a differentiable coordinate transformation that takes the global metric to a local inertial metric (except on a physical singularity).
Figure 8 (right) shows an example of a global coordinate system that fails to satisfy the uniqueness requirement.
About the second requirement (smoothness) in case of Euclidean plane the polar coordinates fulfill the requirement everywhere except that at point O: namely there is a differentiable coordinate transformation that brings the global metric (expressed in polar coordinates) into local inertial metric form (i.e. standard Euclidean form) everywhere except at point O.
Does the above coordinate transformation actually doesn't "count" as differentiable, therefore does not "qualify" polar coordinates as smooth ?
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