You state that the quantum universe is unknowable. I would say there is some limit to how much we can know about it. This limit is due to the cut-off in measurable physics at the Planck or string scale. As one considers scales beneath the string length and then beyond the Planck scale spacetime folds up onto itself in such ways that quantum fluctuations result in closed timelike curves and things that are "paradoxical." This is probably a domain that is fundamentally unobservable.
A rather simple argument can illustrate how this cut-off on the extremely small scale manifests itself on a larger and I think potentially a cosmological scale. The amplitude computed in a path integral is a summation over 3-metrics g
Z = ∫D[g]e^{iS(g)},
where a standard method is to Wick rotate the phase e^{iS(g)} --- > e^{S(g)}. This is a way to get attenuation of high frequency modes, and it is a "bit of a cheat," though at the end one must recover the i = sqrt{-1} and "undo the damage" for the most part. This phase then becomes e^{-GM^2}, which illustrates how the action and entropy are interchangeable. The integral measure is the size of the phase space of the system ~ exp(S). The amplitude is then on the order
Z ~ e^{S}e^{-S} = 1.
This holds universally no matter how large the black hole is. A black hole is a sort of theoretical laboratory for the universe at large, where the universe has a cosmological horizon at r = sqrt{3/Λ}. The implication is there is a limit to what we can possibly observe about the foundations of the universe, which probably touch on the amount of quantum information available with respect to quantum gravity/cosmology.
We have of course two different quantities. The volume of the phase space is equal to the exponential of the entanglement entropy of the system, while the e^{-S} is exponential of the thermal entropy. The amount of information is S_{th} - S_{ent}, so this amplitude is not going to be exactly one. There is some "kernel" to the black hole which corresponds to an elementary unit of information. This means that quantum information is ultimately conserved, and that the number of degrees of freedom for a black hole in spacetime is a constant, regardless of the size of the black hole. It also means that the universe as a whole (here thinking of a toy universe with just a black hole) has a finite limit to its domain of observability.
The application of modal logic is a sort of "boilerplate" to examine causality and locality. Further, my considerations are quantum field theory instead of quantum mechanics. QFT involves operators which act on a Fock space to describe quantum states or QM. So this is an underlying physics. Your work seems to illustrate the "traces" of this sort of underlying QFT in matters of CHSH nonlocality.
The paper by Dzhunushaliev looks interesting. Your work with G2(2), which I am presuming is a split form of G2, focuses on the automorphism of the E8 or octonions. The F4 is a stabilizer of E8 (constant under G2 action). The automorphism on E8 defines an invariant interval on C^4 as a twistor space. This in higher forms, say on the magic square can construct generalizations on H^2 and then O, within the CxO, HxO and OxO hierarchy of the magic square. Generalizing the H^2 twistor space to octonions gives O^2, and scattering amplitudes are functions on copies of OP^1, subject to SL(2,O) = Spin(9,1) transformations. Embedding O^2 in O^3, gives OP^1 as a line in OP^2 and SL(2,O)=Spin(9,1) becomes the subgroup of SL(3,O) = E6(-26), consisting of transformations (collineations) that fix a point in OP^2.
The J^3(O) or O^3 has connections to SO(2,1) and I think this rather erudite stuff connects to anyons on a 2-space plus time constructions. All of this I think is some sort of superselection rule on this sort of theory. The question might then be whether your idea about [0, 1, ∞] as the dessin d'enfant is some sort of category theory on the superselection rules according to curves on Ricci flat spaces, such as (K_3)^2 for E_6 twistor theory.
Cheers LC