DrGreg
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It really is just a coincidence, and DaleSpam has said it all on that subject.Austin0 said:That is a truly amazing and provocative coincidence which has occupied my thoughts since reading it.
1) But having thought about it I can't make the leap from 1 ls/s^2 to 10m/s^2 if the g you are referring to is the local constant. Could you point me towards a reference to how to make this connection?
2) As I understand it g is a local value derived from G which in GR is still a universal constant? so does this mean this applies to G also.
3) Were you possibly being facetious and humerous when you used the term "cosmic coincidence" and that you don't think there is anything coincidental about the relationship whatsoever? That it is actually fully understood.
To do the calculation yourself: 1 ly/y2 is, by definition, the coordinate acceleration (relative to an inertial frame) that would take you from 0 to c in 1 year of coordinate time. (Of course, such a journey isn't physically possible. As your speed approached c, your proper acceleration would approach infinity, which makes the journey impossible to complete.) Nevertheless, you can use the equation v = at, with v = 3 x 108 m/s and t = 365.25 x 24 x 60 x 60 s to calculate the acceleration in m/s2.
Austin0 said:Just as a check; Am I right in thinking that cartesian, polar and Minkowski coordinate systems all work on the assumption of a uniform time metric within any given frame?
ANd that all three are fundamentally euclidean ?
That the Rindler coordinate system assumes a non-uniform time metric and is different from the other three in this regard??
In the example I gave, Cartesian and polar coordinates are two different ways to measure static points in 2D space. Time is not involved, we are just looking at the geometry of static points on a flat piece of paper. It's Euclidean geometry whichever coordinate system you use.
The Minkowski and Rindler coordinates are two different ways to measure events in 2D spacetime (in my example, a cut-down version of 4D spacetime). Specifically "flat" spacetime which means gravity is being ignored. It's "Minkowski geometry" whichever coordinate system you use. Some might call it "Lorentzian geometry". The word "geometry" is now being used in an analogous sense as we are thinking of 2D spacetime as being a 2D geometrical entity. One of the dimensions is now time instead of space, but we can still draw spacetime graphs on a flat 2D piece of paper and look and the geometry of the curves. Only we have to use "Minkowski geometry" instead of "Euclidean geometry" and we have to measure our "pseudo-distance" on the graph using ds2 = dt2 - dx2.
The "non-uniform time metric", as you put it, is analogous to the fact that in 2D Euclidean geometry in polar coordinates you have a "non-uniform angle metric"; when an angle changes by one degree, the distance traveled depends on the radius.
I'm not quite sure what you mean here, but there's a distinction to be drawn between the geometry of space and the the geometry of spacetime. The physical interpretation of the metric of flat (gravity-free) spacetime is that free-falling objects always move at constant velocity relative to any inertial frame. The trajectories of free-falling objects define what a "straight line" (or "geodesic") is in spacetime which in turn determines the spacetime geometry. When you choose Rindler coordinates instead of Minkowski coordinates, it means the coordinate gridlines that you measure with are no longer all straight lines.Austin0 said:Am I wrong in thinking that the geometry of space-time is not a static function and that a non-uniform time metric would imply a non-euclidean geometry as described by the motions of points or particles over time?
You can see a diagram of Rindler gridlines attached to post #9 of this thread.