FallenApple said:
then the object that moves in a curved spacetime isn't really accelerating relative to it's own frame of reference.
Here are a few shortcuts, 'tricks', to remember a few basics of relativity, thanks to experts here, like Dr.Greg, A.T.,bcrowell, Peter Donis and others. You can search 'relativity' and their names here for many details;there may also be FAQ's of interest.
[1] It took Einstein ten years to formulate GR. And he did not know all the math himself; he had help. So it's complicated and takes time to understand, especially the finer points. No one has yet been able to combine GR with the three 'forces' [of the Standard Model of particle physics]; GR is unique. A key aspect of GR is a special geometrical 'curvature'.
[2] Acceleration. To answer your question I quoted in this post, do you feel "acceleration" when you are in free fall? That is, does an accelerometer measure acceleration? No. In contrast, imagine sitting at your computer right now, do you feel a force on your backside? THAT's acceleration in relativity! Just like when you fall down on ice and hit the ground; the 'acceleration' is when you stop and say 'ouch'. That's a different view from Newton's. In GR, you are accelerating when you are not following a 'geodesic' [that's an idealization].
[3] Gravity is a geometrical framework involving very special descriptions of space and time 'distortion', that is, special types of curvature. Consider everyday flat graph paper with a square grid pattern and a path of some object, a 'worldine'...a path through space and time, say 'x' versus 't', a plot of d=vt if you like .
[a] A flat graph paper with square grids frame is inertial motion in SR. The object moves in a straight line.
[These are the "Minkowski' flat coordinates of 'spacetime' of SR; Even Einstein did not at first realize how important it was; Herman Minkowski, a I think Einstein's former math professor pointed it out and Einstein wisely adopted it.]
If you accelerate in SR, the grid squares on the flat graph now appear distorted. That is, a non inertial [accelerating] observer will draw a curved grid on flat graph paper.
[This is why the speed of light in SR looks different from 'c' to an accelerating observer: To the accelerating observer the light appears to be crossing non square, different size grids!.
[c] With gravity, the graph paper reference frame itself is curved in a special way, NOT like at the end of AT's posted illustration. [I'm not sure what the cylinder and cone are supposed to illustrate there...that is not gravity.] This special curvature of GR manifests in such a way that the graph paper cannot be flattened out, say on a table, without further distorting it...visualize a partially crumpled graph paper for example. Gravitational curvature is that special kind of 'distortion', not a rolled up version of flat graph paper into either a cylindrical or a conical shape.
FallenApple said:
So is it like a generalized version of Newton's law of intertia?
From my notes of an earlier discussion:
Dalespam: One of the great theoretical accomplishments of GR is to unify inertia and gravity. Prior to Einstein it was recognized that the passive gravitational mass was equal to inertial mass, but it was not known why. Afterwards, it became clear that they must be equal since gravitation is inertia in curved spacetime