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We study the Vaidya black hole surrounded by the exotic quintessence-like,phantom-like and cosmological constant-like fields by means of entropicconsiderations. Explicitly, we show that for this thermodynamical system, therequirement for the identification of D-bound and Bekenstein entropy bound canbe considered as a thermodynamical criterion by which one can rule out thequintessence-like and phantom-like fields, and prefer the cosmological constantas a vi{\th}able cosmological field.

D-bound and Bekenstein Bound for the Surrounded Vaidya Black Hole