A new mass scale, implications on black hole evaporation and holography

We consider a new mass scale $M_T=({\mathrm{\hslash }}^2\sqrt{\mathrm{\Lambda }}\mathrm{/}G{)}^{1\mathrm{/}3}$ constructed from dimensional analysis by using $G$, $\mathrm{\hslash }$ and $\mathrm{\Lambda }$ 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 $M_T^{\mathrm{\prime }}=c(\mathrm{\hslash }\mathrm{/}{G}^2\sqrt{\mathrm{\Lambda }}{)}^{1\mathrm{/}3}$ 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.