We look in Euclidean R 4 for associative star products realizing the commutation relation [ x μ , x ν ] = i Θ μ ν ( x ) , where the noncommutativity parameters Θ μ ν depend on the position coordinates x. We do this by adopting Rieffel's deformation theory (originally formulated for constant Θ and which includes the Moyal product as a particular case) and find that, for a topology R 2 × R 2 , there is only one class of such products which are associative. It corresponds to a noncommutativity matrix whose canonical form has components Θ 12 = − Θ 21 = 0 and Θ 34 = − Θ 43 = θ ( x 1 , x 2 ) , with θ ( x 1 , x 2 ) an arbitrary positive smooth bounded function. In Minkowski space–time, this describes a position-dependent space-like or magnetic noncommutativity. We show how to generalize our construction to n ⩾ 3 arbitrary dimensions and use it to find traveling noncommutative lumps generalizing noncommutative solitons discussed in the literature. Next we consider Euclidean λ ϕ 4 field theory on such a noncommutative background. Using a zeta-like regulator, the covariant perturbation method and working in configuration space, we explicitly compute the UV singularities. We find that, while the two-point UV divergences are nonlocal, the four-point UV divergences are local, in accordance with recent results for constant Θ.
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