  We investigate both the interacting and non-interacting R\'{e}nyi Holographic
Dark Energy (RHDE) models in DGP brane world framework. Cosmological parameters
and their evolutions are probed to obtain realistic cosmological models. We
note that both the models accommodate the present accelerating phase of
expansion with the observed dark energy density. Classical stability of the
cosmological model and $Om$- diagnostic are also studied to test the
suitability of the cosmological models obtained in the presence of RHDE in DGP
braneworld.
