  Here, we report the new detection of three shock fronts using archival
\textit{Chandra} X-ray observations in Abell 1914, which also hosts a radio
halo, a radio phoenix, and a head-tail galaxy. In this study, we report the
X-ray shock front at the position of the radio phoenix, which further
strengthens the scenario that radio phoenix traces old plasma that gets lit up
when compressed by shock passage. We further analyze the thermodynamic
structure of the cluster in detail. We create temperature maps of A1914 using
three different techniques, Adaptive Circular Binning (ACB), Weighted Voronoi
Tessellations (WVT), and Contour binning (Contbin) method. These thermodynamic
maps, along with the pseudo pressure and the pseudo entropy maps for the
cluster, are evidence of disturbed morphology produced by multiple merger
events. These merger events create cluster-wide turbulence, which may
re-accelerate the relativistic particles and result in a radio halo within the
cluster. Further, comparing X-ray and radio images reveals that the radio halo
is contained within two X-ray shock fronts. Our analysis suggests that A1914
has both equatorial shock and axial shock within the cluster's ICM. We proposed
a dual merging scenario based on the shock position and analysis of the
thermodynamic maps obtained from the deeper \textit{Chandra} X-ray
observations.
