  We explore some general consequences of a consistent formulation of
relativistic quantum field theory (QFT) on the Groenewold-Moyal-Weyl
noncommutative versions of Minkowski space with covariance under the twisted
Poincare' group of Chaichian et al. [12], Wess [44], Koch et al. [31], Oeckl
[34]. We argue that a proper enforcement of the latter requires braided
commutation relations between any pair of coordinates $\hat x,\hat y$
generating two different copies of the space, or equivalently a $\star$-tensor
product $f(x)\star g(y)$ (in the parlance of Aschieri et al. [3]) between any
two functions depending on $x,y$. Then all differences $(x-y)^\mu$ behave like
their undeformed counterparts. Imposing (minimally adapted) Wightman axioms one
finds that the $n$-point functions fulfill the same general properties as on
commutative space. Actually, upon computation one finds (at least for scalar
fields) that the $n$-point functions remain unchanged as functions of the
coordinates' differences both if fields are free and if they interact (we treat
interactions via time-ordered perturbation theory). The main, surprising
outcome seems a QFT physically equivalent to the undeformed counterpart (to
confirm it or not one should however first clarify the relation between
$n$-point functions and observables, in particular S-matrix elements).
  These results are mainly based on a joint work [24] with J. Wess
