  This paper discusses noncommutative-geometry wormholes in the context of a
cosmological model due to Sung-Won Kim. An ansatz suggested by the
Friedmann-Lemaitre-Robertson-Walker (FLRW) model leads to the assumption that
the matter content can be divided into two parts, a cosmological part depending
only on time and a wormhole part depending only on space. These assumptions are
sufficient for deriving a complete zero-tidal force wormhole solution. The
wormhole is evolving due to the scale factor in the FLRW model; it is
restricted, however, to the curvature parameters $k=0$ and $k=-1$. Unlike
previous models, the noncommutative-geometry background affects both the
wormhole part and the cosmological part of the solution.
