  We examine the quasi normal modes of Ellis-Bronnikov wormholes embedded in a
warped five dimensional braneworld background and compare with it's four
dimensional counterpart. These scalar quasi normal frequencies are obtained
using the WKB formula, Prony method and the direct integration method. The
signature of the warped extra dimension shows up as two distinct quasi normal
ringing era, characterised by two distinct dominant quasi normal modes.
Features of the latter region are similar to that observed earlier for massive
scalar field in black hole background. We also discuss the how steepness of the
neck of the wormhole effects the quasi normal frequencies.
