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This work is the reconstruction of the interaction rate of holographic darkenergy whose infrared cut-off scale is set by the Hubble length. We havereconstructed the interaction rate between dark matter and the holographic darkenergy for a specific parameterization of the effective equation of stateparameter. We have obtained observational constraints on the model parametersusing the latest Type Ia Supernova (SNIa), Baryon Acoustic Oscillations (BAO)and Cosmic Microwave Background (CMB) radiation datasets. We have found thatfor the present model, the interaction rate increases with expansion andremains positive throughout the evolution. For a comprehensive analysis, wehave also compared the reconstructed results of the interaction rate with otherwell-known holographic dark energy models. The nature of the decelerationparameter, the statefinder parameters and the dark energy equation of stateparameter have also been studied for the present model. It has been found thatthe deceleration parameter favors the past decelerated and recent acceleratedexpansion phase of the universe. It has also been found that the dark energyequation of state parameter shows a phantom nature at the present epoch.

Reconstruction of interaction rate in Holographic dark energy model with Hubble horizon as the infrared cut-off