  We construct scalarized wormholes with a NUT charge in higher curvature
theories. We consider both Einstein-scalar-Gauss-Bonnet and
Einstein-scalar-Chern-Simons theories, following a recent paper by Brihaye et
al. [1], where spontaneously scalarised Schwarzschild-NUT solutions were
studied. By varying the coupling parameter and the scalar charge we determine
the domain of existence of the scalarized nutty wormholes, and their dependence
on the NUT charge. In the Gauss-Bonnet case the known set of scalarized
wormholes [2] is reached in the limit of vanishing NUT charge. In the
Chern-Simons case, however, the limit is peculiar, since with vanishing NUT
charge the coupling constant diverges. We focus on scalarized nutty wormholes
with a single throat and study their properties. All these scalarized nutty
wormholes feature a critical polar angle, beyond which closed timelike curves
are present.
