  In this paper, we investigate the statefinder, the deceleration and equation
of state parameters when universe is composed of generalized holographic dark
energy or generalized Ricci dark energy for Bianchi I universe model. These
parameters are found for both interacting as well as non-interacting scenarios
of generalized holographic or generalized Ricci dark energy with dark matter
and generalized Chaplygin gas. We explore these parameters graphically for
different situations. It is concluded that these models represent accelerated
expansion of the universe.
