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In this work, we have studied accretion of dark energy (DE) onto Morris-Thorne wormhole with three different forms, namely, holographic dark energy,holographic Ricci dark energy and modified holographic Ricci dark energy .Considering the scale factor in power-law form we have observed that as theholographic dark energy accretes onto wormhole, the mass of the wormhole isdecreasing. In the next phase we considered three parameterization schemes thatare able to get hold of quintessence as well as phantom phases. Without anychoice of scale factor we reconstructed Hubble parameter from conservationequation and dark energy densities and subsequently got the mass of thewormhole separately for accretion of the three dark energy candidates. It wasobserved that if these dark energies accrete onto the wormhole, then forquintessence stage, wormhole mass decreases up to a certain finite value andthen again increases to aggressively during phantom phase of the universe.

Can Holographic dark energy increase the mass of the wormhole?