An integral kernel representation for the commutative $$\star $$
⋆
-product on curved classical spacetime is introduced. Its convergence conditions and relationship to a Drin’feld differential twist are established. A $$\star $$
⋆
-Einstein field equation can be obtained, provided the matter-based twist’s vector generators are fixed to self-consistent values during the variation in order to maintain $$\star $$
⋆
-associativity. Variations not of this type are non-viable as classical field theories. $$\star $$
⋆
-Gauge theory on such a spacetime can be developed using $$\star $$
⋆
-Ehresmann connections. While the theory preserves Lorentz invariance and background independence, the standard ADM $$3+1$$
3
+
1
decomposition of 4-diffs in general relativity breaks down, leading to different $$\star $$
⋆
-constraints. No photon or graviton ghosts are found on $$\star $$
⋆
-Minkowski spacetime. $$\star $$
⋆
-Friedmann equations are derived and solved for $$\star $$
⋆
-FLRW cosmologies. Big Bang Nucleosynthesis restricts expressions for the twist generators. Allowed generators can be constructed which account for dark matter as arising from a twist producing non-standard model matter field. The theory also provides a robust qualitative explanation for the matter-antimatter asymmetry of the observable Universe. Particle exchange quantum statistics encounters thresholded modifications due to violations of the cluster decomposition principle on the nonlocality length scale $$\sim 10^{3-5} \,L_P$$
∼
10
3
-
5
L
P
. Precision Hughes–Drever measurements of spacetime anisotropy appear as the most promising experimental route to test deformed general relativity.