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I can't comment upon the muonic atom result which got the radius of the proton adjusted. I will offer my suggestion that the large muon has a small orbit and these results reflect the interaction of the muon with the proton. So the perturbation may be reflected by this result. To ferret out the problem requires some very complicated QED calculations with a quark or parton model of the proton.
The fluid properties of the quark-gluon plasma is interpreted as an AdS_4 ~ QCD result. In effect the quark gluon has properties of a BTZ black hole in the anti de Sitter spacetime. There is then some parameter that depends on energy, so that at low energy the quark gluon plasma has properties of a black hole with very weak gravity, but as the energy is scaled up the QCD plasma becomes a real black hole with strong gravity. Nastase and others have written on this.
The value of the cosmological constant means there is some field flux across the Dp-brane of the cosmology that counters the vacuum energy. The AdS has negative Gaussian curvature, which counters the Ricci curvature on the S^5. In the AdS_5xS^5 the boundary of AdS_5 = ∂AdS_5 ~ CFT_4. The AdS_5 has negative Gaussian curvature, which is from a 5-form which has a positive curvature on the S^5. On the boundary the gravitational curvature is zero. So problem involves the incidence of these curvature fluxes on the Dp-branes in the presence of these spaces.
My understanding is that since Bohm QM does not involve Hilbert space, the whole thing lives in configuration space, it is difficult to model the production of particles. One can well enough derive a Bohm version of the Klein-Gordon equation, or the Dirac equation, and even the Maxwell equations. The problem comes when you couple them together. It is difficult to describe the generation of photons, which are massless, and from what I know up to now it is not possible to describe the pair production of particles with some mass --- such as e-e^ pairs.
Cheers LC