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The dark energy problem is analyzed from the viewpoint of the time-varying cosmological term. It is demonstrated that, at least within the scope of the holographic principle, an experimental value of the vacuum energy density may be derived and may be tested quite well with a new small parameter arising in a quantum theory with the fundamental length on the order of Planck's length. Besides, within a theory proclaiming the existence of such fundamental length a high-energy deformation of thedoi:10.5923/j.ijtmp.20110101.01 fatcat:bjhiujijm5hxtd2gdfyohcc2ba