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Hi Marcoen and thanks for the excellent questions:
(1) Perhaps I should state this as actually three different functions f1, f2 and C. I do mean that C is a constant (i.e. a number) and not a function of x (i.e. C(x), a constant can still be integrated, so perhaps when I referred to it as a constant function this was misconstrued as meaning it to be a linear constant function of x, which it is not). A very elementary part of calculus, not something which stands out. The point is that from the answer alone, which would just be area, there is no way to tell whether I used an integration of f1 over x1 to x2 or the integration of C-f2. If one finds the antiderivative of a function, there exists an arbitrary constant of integration which could have any value.
I use this specific example, in that if the cosmological constant is a constant of integration (sometimes called the unimodular approach), then it is a bit of a coincidence that one of the biggest paradoxes about it is that it should be extremely large (according to QFT) but that empirically it appears to be rather tiny. In my example, the constant C could be extremely large or it could be zero and there is no way from anti-differentiation to tell which.
(2) Why would my equation be an improvement over Einstein's tensor G? It could also be fairly asking whether I am making the equation more difficult. To answer this question fully, it might be helpful if we consider a model of a cosmological fluid (see the Dark Energy Task Force report on the use of these). With the modified EFE, there is no known way to put in the estimated value of the cosmological constant (10120 higher than observed) and also find a mechanism which makes it very small. However, by using the alternate equation I propose, a full theoretical value of the "vacuum" could be put in. Suppose then there is matter present at a point in this vacuum. If we model this particle as a reduction in the density of this cosmological fluid, the Luv would be equated to the stress energy tensor of the remaining density kTresuv. Since this constant and remaining stress energy tensor together are mathematically equivalent to the Einstein tensor/stress energy tensor of matter, it should approximate Newtonian gravity, although calling that gravity "attractive" would be qualitatively incorrect. The main point of this though, is that it appears that it would not model it exactly, since at larger radii the Omega term would increase linearly to a point where the gravitational vector switches direction from an apparent attraction to a repulsion. Whether this matches what we empirically observe I do not yet know, but there are too many coincidences in the formation of field theory, action at a distance, GR and now a linear accelerating expansion that has been tied to the cosmological constant to not be suspicious. If this model gives us a more accurate picture of macro gravitational effects, I would also become very concerned about how abstract these cosmological fluid models actually are.