  We consider a new mass scale $M_{T}=(\hbar^{2}\sqrt{\Lambda}/G)^{1/3}$
constructed from dimensional analysis by using $G$, $\hbar$ and $\Lambda$ and
discuss its physical interpretation. Based on the Generalized Uncertainty
Relation, a black hole with age comparable to the universe would stop radiating
when the mass reaches a new mass scale
$M'_{T}=c(\hbar/G^{2}\sqrt{\Lambda})^{1/3}$ at which its temperature
corresponds to the mass $M_{T}$. Black hole remnants could have masses ranging
from a Planck mass to a trillion kilograms. Holography persists even when the
uncertainty relation is modified to the Minimum Length Uncertainty
Relation~(MLUR). The remnant black hole entropy is proportional to the surface
area of the black hole in unit of the Planck area in arbitrary noncompact
dimensions.
