  Internal gravity waves (IGWs) are likely to cause mixing in stellar
interiors. Studies show that the mixing by these waves changes drastically
across age and mass (Varghese et al. 2023, arXiv:2211.06432). Here, we study
the effect of rotation on this wave mixing by considering a 7 M$_{\odot}$ model
at ZAMS and midMS. We compare the mixing profiles at a range of rotation rates
($1\times 10^{-5}$, $2\times 10^{-5}$, $3\times 10^{-5}$, $4\times 10^{-5}$ and
$1\times 10^{-4}$ rad.s$^{-1}$) and observe that the mixing decreases with
decreasing Rossby number. This can be attributed to the effect of rotation on
convection which influences the amplitude with which the waves are excited near
the convective-radiative interface.
