Testing for the positive presence of quantum fields essentially amounts to verifying that particles physics works. The field itself is a mathematical construct; the physical manifestations of the field include particles and vacuum fluctuations. We know that each of these things exist here on Earth. In the same way that we generally assume the extension of the laws of physics to apply elsewhere in the universe, we do so for the quantum field.
Now, the statement that the quantum vacuum does not gravitate is central to understanding the dark energy problem. It is true that a naive summation of vacuum fluctuations up to the Planck scale leads to an enormous disparity with the observed expansion rate. However, it is not particularly obvious that we should be simply summing the vacuum contributions of each field to compute the total gravitational vacuum energy density. In flat spacetime, we subtract off the infinity on the grounds that it is unphysical. There are, however, instances where the vacuum energy does physically manifest itself, e.g. the Lamb shift and the Casimir effect. Both of these involve restricted dimensions: the quantum vacuum only shows itself when it is in some sense confined (specifically, when the vacuum modes get discretized). We might expect something similar to happen in GR.
While it's true that the energy content of the spacetime causes gravitation, it is generally assumed that the divergent parts of the stress tensor should still be subtracted. The complicating issue in GR is the lack of a unique vacuum: what vacuum do we use?? How do we isolate uniquely the divergent parts of the stress tensor? This has lead to the enormous field of research focused on renormalizing the stress energy tensor in curved spaces: it is complicated and as far as I know, no perfectly satisfactory (generally applicable) formulation has been found (see the excellent text by Birrell and Davies for details).
In analogy with the Casimir effect, Ford (
http://prd.aps.org/abstract/PRD/v11/i12/p3370_1) sidestepped the above difficulties by looking at situations where the gravitational field was a small perturbation on Minkowski space. Here, the vacua are unique, the stress tensor is calculated for the perturbed spacetime, and then the perturbation is smoothly turned off and Minkowski space is obtained. If the difference between the perturbed stress tensor and that of Minkowski is finite and cut-off independent, then Ford argues
this difference is the physical vacuum energy. This is sensible, but it only works in a very restricted set of circumstances.
So, it's an open and complicated problem. That a naive summation of vacuum fluctuations does not happen to agree with the observed expansion signals to me that this is not the right way to do the calculation. It does not necessarily imply to me that vacuum energy does not gravitate, or that, as per your suggestion, that quantum fields simply don't exist elsewhere in the universe.