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We obtain a \textit{novel} model of oscillating non-singular cosmology on thespatially flat Randall-Sundrum (RS) II brane. At early times, the universe isdominated by a scalar field with an inflationary emergent potential$V(\phi)=A(e^{B\phi}-1)^2$, $A$ and $B$ being constants. Interestingly, we findthat such a scalar field can source a non-singular bounce, replacing the bigbang on the brane. The turnaround again happens naturally on the branedominated by a phantom dark energy (favoured by observations\cite{E1,E2,E3} atlate times), thus avoiding the big rip singularity and leading upto thefollowing non-singular bounce via a contraction phase. There is a smoothnon-singular transition of the brane universe through both the bounce andturnaround, leading to alternate expanding and contracting phases. This is the\textit{first} model where a single braneworld of positive tension can be madeto recycle as discussed in details in the concluding section.

A novel model of non-singular oscillating cosmology on flat Randall-Sundrum II braneworld