Some worldlines satisfy the geodesic equation, others don't. The ones which do are geodesics. It's not true that GR cannot incorporate other forces of nature
This is a matter of terminology, but I would maintain that a physical theory is defined by its equations of motion, and that GR is defined by the Einstein equation(s); and since the other forces do not appear in the Einstein equation(s), they are not part of GR. (There is no question of being able to incorporate them; the theory either does or does not incorporate them.) If you're working with Maxwell's equations in curved spacetime, you're not working in GR; you're working in a hybrid of GR and Maxwell's theory.
Thus defined, GR itself does not (as far as I know) allow non-geodesic paths to be worldlines. (An Einstein-Maxwell hybrid theory, on the other hand, might; but I would be tempted to suspect in that case that it isn't formulated "properly".)
The point I was making is that representing spacetime as a Lorentzian manifold (even a Lorentzian manifold with arbitrary curvature) is insufficient (and unnecessary) to get "no privileged reference frame". What that requires is that the laws in the theory are formulated in such a way that they do not presume anything about the reference frame in which they hold.
But that is the same thing, only expressed in old-fashioned physicist's language instead of modern mathematician's language. If you translate "the laws in the theory are formulated in such a way that they do not presume anything about the reference frame in which they hold" into modern mathematician's language, what you get is "the equations of motion must be expressed in terms of objects which are well-defined on a manifold (of the appropriate type)".
It is true that one can change coordinates so that the metric at a point is Minkowski. This is what people usually mean when they talk about using a locally flat coordinate frame. But the metric reducing to Minkowski at a point does not mean that the curvature at that point vanishes. Curvature has to do with the second derivatives of the metric.
I could hardly have said it better myself. The ability to use a locally flat coordinate system at a point (regardless of the value of the Riemann tensor at that point) is all that
you could never tell the difference between firing your rocket to accelerate through flat spacetime, and firing your rocket to stay in the same place in curved spacetime.
means.
I could hardly have said it better myself. The ability to use a locally flat coordinate system at a point (regardless of the value of the Riemann tensor at that point) is all that
you could never tell the difference between firing your rocket to accelerate through flat spacetime, and firing your rocket to stay in the same place in curved spacetime.
means.
I don't see how it could mean that. Rockets are extended objects, as are people. While we can always find coordinates that make the metric Minkowski at a single point, it is not true that we can always find coordinates that make the metric Minkowski over a finite region, no matter how small.
Today's post, Mach's Principle: Anti-Epiphenomenal Physics was originally published on 24 May 2008. A summary (taken from the LW wiki):
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