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A so called "power-law entropy-corrected holographic dark energy" (PLECHDE)was recently proposed to explain the dark energy dominated universe. This modelis based on the power-law corrections to black hole entropy which appear indealing with the entanglement of quantum fields between inside and outside ofthe horizon. In this paper, we suggest a correspondence between interactingPLECHDE and tachyon, quintessence, K-essence and dilaton scalar field models ofdark energy in a non-flat FRW universe. Then, we reconstruct the potentialterms accordingly, and present the dynamical equations which describe theevolution of the scalar field dark energy models.

Scalar Field Reconstruction of Power-Law Entropy-Corrected HDE