  In this paper we constructed a semi-realistic cosmological model in a dynamic
domain wall framework. Our universe is considered to be a (3+1) dimensional
dynamic domain wall in a higher dimensional Einstein-Maxwell-Born-Infeld
background. One of our interesting outcomes from the effective Hubble equation
for the domain wall dynamics is that it contains an additional component of
"dark matter" which is induced from the charge of the bulk Born-Infeld gauge
field. In this background spacetime we have studied the cosmological dynamics
of the domain wall. In addition to the Born-Infield gauge field if we consider
additional pure gauge field, a non-singular bounce happens at the early stage
with a smooth transition between contracting and expanding phase.
