CycoFin said:
You say that even we have RHS stress-energy T zero, LHS Einstein tensor G is not?
No; I am saying that the Einstein tensor being zero does
not mean "zero apples" or "zero oranges". It means something more like "the rate of change of the rate of changes of apples plus the rate of change of the rate of change of oranges is zero", and nine more equations of that sort. The fact that a bunch of derivatives of something add up to zero does not require that something itself to be zero. And gravity is the "something" here, so this is just saying that the Einstein tensor being zero is not the same as gravity being zero.
CycoFin said:
we have G = 0, I don't disagree this and metric explanation of gravity makes sense and this have been very successfully tested.
And these
are tests of the EFE, because, once again, the LHS of the EFE is not just a simple expression whose value we test to be zero; it's a combination of a bunch of derivatives of different things, and we don't measure the combination, we measure the derivatives separately, so we can test whether they add up to zero as the EFE predicts. That's a valid test.
CycoFin said:
surely there must be some experimental test results so we can write G = constant * T, where T is nonzero energy-stress tensor.
There are, but they're indirect. The sorts of experimental tests you need here are tests of the structure of matter, but it's difficult to find pieces of matter where relativistic effects are significant in determining its structure--i.e., where the difference between the predictions of GR and the predictions of Newtonian gravity are significant. Nothing in our solar system even comes close: Newtonian gravity is sufficient to explain the internal structure of all ordinary objects, and of the Sun and all the planets and other bodies in the solar system.
The kinds of matter (other than what we model in cosmology) for which relativistic effects are significant are, basically, white dwarfs, neutron stars, black holes (these aren't exactly "matter", but they are formed from collapsing matter), and supermassive stars. There aren't any such objects nearby, so we can only observe them indirectly, from far away, hence our observational tests of GR regarding the internal structure of such objects are still very rough.
However, I don't understand why you leave out cosmology here; the cosmological models we use to accurately match many observations, such as the properties of the CMBR and the curvature in the Hubble diagram, certainly require a nonzero stress-energy tensor and are valid tests of GR with a nonzero RHS of the EFE.
atyy said:
The analogy is more like
apples - oranges = 0.
I'm not sure even this conveys it, because "apples" and "oranges" here correspond to different metric coefficients, and the EFE contains derivatives of those. See above.