I really have to object to this.
The experiments completely verify GR and the associated equations that describe the motion of light and matter under gravity.
Now please tell me where the curvature of spacetime enters into the equations of GR. Show me specifically where this occurs because when I studied this I saw nothing of the sort. The experiments verify GR – and contrary to popular belief GR has nothing to do with the curvature of spacetime. The rubber sheet analogy is great for conveying the effects (such as gravity waves), but terrible at representing what the equations actually say.
I have to admit, I am very, very surprised and confused by your question. You have taken a course in GR, and I haven't, so maybe I am about to embarrass myself.....so please correct me if I'm wrong here.....but everything I have ever heard of GR and special relativity is all about the geometry of space(time).
Describing the motions of anything requires you to specify the geometry of space, I don't see how you can calculate position or velocity or anything if you don't specify this (I suppose you could things like energies). This is true in everything, classical mechanics, electromagnetism, etc. however normally the space is "flat" so we don't always explicitly deal with this.
In other words if I measure the position of two points in space according to my chosen coordinate frame, how do I calculate the distance between the two points? In classical mechanics, and electromagnetic dynamics and Special Relativity this is encoded mathematically by the metric tensor. In a "flat" 3D space (the usual kind) the distance S we are interested in is calculated by the Pythagorean theorem, S^2 = X^2 + Y^2 + Z^2 where S is the distance from the origin (0,0,0) and X,Y,Z are the coordinates of the point in question, and in this case the metric tensor is just an all-zero matrix with 1's along the diagonal (I'm ignoring the time-coordinate). In a different space the metric tensor would be different, perhaps with off-diagonal elements and the same point at X,Y,Z would NOT be measured to be distance S from the origin, as it was in the "flat" space according to the Pythagorean theorem.
Now, taking a cursory look at the Wiki articles on GR, apparently the
solutions to Einstein's equations are metrics. Same with this
U. Cal. Riverside intro. to GR:
General relativity explains gravity as the curvature of spacetime. It's all about geometry. The basic equation of general relativity is called Einstein's equation. In units where
, it says
(1)
It looks simple, but what does it mean? Unfortunately, the beautiful geometrical meaning of this equation is a bit hard to find in most treatments of relativity. There are many nice popularizations that explain the philosophy behind relativity and the idea of curved spacetime, but most of them don't get around to explaining Einstein's equation and showing how to work out its consequences. There are also more technical introductions which explain Einstein's equation in detail -- but here the geometry is often hidden under piles of tensor calculus.
So I am at a complete loss as to why you are saying it has nothing to do with the geometry of space. As I understand, you are ultimately
solving for that little "g" character with two subscripts *edit: which is related to the big "G" * the spacetime metric, which is a second-rank tensor (a matrix) with four columns (t,x,y,z). This little guy gave me some headaches in classical mechanics and showed up again in electrodynamics and special relativity. However, when I took those courses g was
given by its value for an assumed flat spacetime.
In other words, given some physical scenario in which you make approximations about mass and energy, you use Einstein's equations to find the metric (or curvature) of space, and that lets you ultimately calculate things as simple as distances. And the metric of space is not flat in all but the simplest situations......the simple, practical consequence of this is you set up a coordinate system, you carefully measure the X,Y,Z position of some point, then you carefully measure its distance from the origin S, and you find the Pythagorean theorem is not accurate, S^2 does not = X^2 + Y^2 + Z^2. The same thing happens in curved 1D or 2D space, this is curved 3D space but it's difficult to picture it in your mind.
Honestly, I feel really awkward because I am supposed to be a physicist (*edit: someday anyway) and really know this stuff, but I have a gap in my education where I haven't studied GR, so please by all means tell me what it was you solved for/calculated when you studied it. At the UCR site they make some simplifying assumptions and then use Einstein's equation to
derive the metric of flat spacetime, but of course flat spacetime is only the solution in that special/simple case.\
*edit: To be a little more specific: the Pythagorean theorem is a special case (flat space) of a more general case (non-flat space) : S^2 = G1*(X^2) + G2*(Y^2) + G3*(Z^2), in flat space G1 = 1 and G2 = 1 and G3 = 1, so you don't even write it out explicitly. But this is only true in flat space, that is, it is only true when the matrix g (the space metric) is all zeroes with only 1's along the diagonal. If this were always true (space is always flat) then Einstein's equation wouldn't make sense, G would simply be given by g (and I believe some tensor related to curvature) and would not depend on momentum or energy (contained in the tensor T).