The ability to faithfully reproduce the effect of axial rotation on fully d
eveloped turbulent pipe how is investigated using a low-Reynolds-number, se
cond-moment closure model. In particular, the impact of the pressure-strain
model is scrutinized by adopting both linear and nonlinear models. Near-wa
ll effects are modeled by elliptic relaxation, and model predictions are ve
rified against direct numerical simulations as well as experimental results
, The results suggest that pressure-strain models cubic in the Reynolds str
esses seem unsuitable for this particular case, whereas the best overall pe
rformance is obtained by a model that retains terms quadratic in the Reynol
ds stress tensor. However, the stabilizing effect of the imposed axial rota
tion on the turbulence is in general overpredicted by the models.