Recently, the Heisenberg’s uncertainty principle has been extended to
incorporate the existence of a large (cut-off) length scale in de Sitter or
anti-de Sitter space, and the Hawking temperatures of the Schwarzshild-(anti)
de Sitter black holes have been reproduced by using the extended uncertainty
principle. I generalize the extended uncertainty to the case with an absolute
minimum length and compute its modification to the Hawking temperature. I
obtain a general trend that the generalized uncertainty principle due to the
absolute minimum length always'' increases the Hawking temperature, implying faster’’ decay, which is in conformity with the result in the asymptotically
flat space. I also revisit the ``black hole-string’’ phase transition, in the
context of the generalized uncertainty principle.

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