DaleSpam said:
Maybe you can be more explicit. Please show the full tensorial expressions for precisely the measurements that you are considering. From what you have written here I still don't see anything that I haven't already rebutted.
Okay... Only there's a bit of the way you'll have to do by yourself. Which is to realize:
1) all of this is done on one and same manifold M, in a neighborhood of one 4-point e, so we pick one set of coordinates around e and write everything in the basis of tangent vectors.
2) not everything that is measured is a tensor, so the best we can do is to show their components in the chosen basis.
Measurement #1: interferometry; yields g_{ab}, the components of the fundamental metric;
Measurement #2: gravimetry; yields \Gamma^a_{bc} the components of the connection in the chosen basis, possibly under the postulate that the connection is symmetric.
These are smooth fields, meaning that we imagine we could get a continuous record of these quantities with arbitrary precision all along any finite set of paths from e to some other point e', and numerically compute derivatives, to any order and with arbitrary precision as well.
What properties the result could verify is anyone's guess at this time; so let's speculate
1) we compute the Ricci tensor: R_{ab} =<br />
\partial_{d}{\Gamma^d_{ba}} - \partial_{b}\Gamma^d_{da}<br />
+ \Gamma^d_{de} \Gamma^e_{ba}<br />
- \Gamma^d_{be}\Gamma^e_{da} <br /> and discover that it is symmetric,
2) we compute its partial derivatives and discover that they verify R_{db}\Gamma^d_{ca} + R_{da}\Gamma^d_{cb} - \partial_{c}{R_{ab}} = R_{ab}\phi_{c}<br /> for a certain set of components \phi_{c}, which are those of a tensor by the way since the LHS is a covariant derivative;
3) taking derivatives again, we discover that \phi is curl-free: \partial_{b}{\phi_{a}} = \partial_{a}{\phi_{b}} <br />, so that \phi is the 4-gradient of some scalar field for which we choose the expression e^{-\rho},
4) we numerically integrate \phi to obtain \rho;
then, with but moderate amazement, we'll find that <br />
\Gamma^a_{bc}=\frac{1}{2}h^{ad} \left(<br />
\partial_{b}h_{dc} + \partial_{c}h_{db} - \partial_{d}h_{bc}\right)\, <br /> where h is defined as h_{ab}=R_{ab} / \rho and of course h^{ab}h_{bc}=\delta^a_c
The whole point being that none of the hypotheses in the above sorites mentions g. In other words, h, the gravitational potential, can obtain from the \Gamma^a_{bc}'s alone. It is a peculiarity of Einsteinian GR that it be equal to g.