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Jonathan Scott said:There are many ways to use Mach's Principle, and I do not see any need to assume anything non-local (that is, involving "faster than light" communication or direct "action at a distance").
Well, at first glance (or first think), Mach's principle is saying that only relative motion is meaningful. So rotation or acceleration of a single object doesn't mean anything--the only meaningful notion is rotation or acceleration relative to some other object (the "fixed stars", for example). But if there is no action-at-a-distance, then how can the rotation or non-rotation of distant stars be relevant here? The answer given by General Relativity is that spacetime itself is an entity that provides a reference for acceleration or rotation. Rotation or acceleration is not measured relative to the distant stars, but relative to the local geodesics determined by the metric tensor. So I would say that GR fails to satisfy Mach's principle.
A way to see this is that Mach's principle would say that without the fixed stars to provide a reference for acceleration and rotation, a single rigid object cannot be said to be rotating. However, there are solutions of GR that consist of a single rotating star in an otherwise empty universe. This is a different solution than a single nonrotating star. So rotation makes a difference, even in the absence of distant stars to provide a reference for rotation.