  In this paper, we carry out a detailed analysis of the M1.6 class eruptive
flare occurring in NOAA active region 13078 on 2022 August 19. The flare is
associated with a fast coronal mass ejection (CME) propagating in the southwest
direction with an apparent speed of $\sim$926 km s$^{-1}$. Meanwhile, a shock
wave is driven by the CME at the flank. The eruption of CME generates an
extreme-ultraviolet (EUV) wave expanding outward from the flare site with an
apparent speed of $\geq$200 km s$^{-1}$. As the EUV wave propagates eastward,
it encounters and interacts with the low-lying adjacent coronal loops (ACLs),
which are composed of two loops. The compression of EUV wave results in
contraction, expansion, and transverse vertical oscillations of ACLs. The
commencements of contraction are sequential from western to eastern footpoints
and the contraction lasts for $\sim$15 minutes. The speeds of contraction lie
in the range of 13$-$40 km s$^{-1}$ in 171 {\AA} and 8$-$54 km s$^{-1}$ in 193
{\AA}. A long, gradual expansion follows the contraction at lower speeds.
Concurrent vertical oscillations are superposed on contraction and expansion of
ACLs. The oscillations last for 2$-$9 cycles and the amplitudes are $\leq$4 Mm.
The periods are between 3 to 12 minutes with an average value of 6.7 minutes.
The results show rich dynamics of coronal loops.
