A note on the black hole information paradox in de Sitter spacetimes

Physics – High Energy Physics – High Energy Physics - Theory

Scientific paper

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4 pages, 1 figure. v3: refereed version

Scientific paper

10.1088/0253-6102/52/1/17

The possibility of stable or quasi--stable Planck mass black hole remnants as solution to the black hole information paradox is commonly believed phenomenologically unacceptable: since we have to expect a black hole remnant for every possible initial state, the number of remnants should be infinite. This would lead to remnant pair production in any physical process with a total available energy roughly exceeding the Planck mass, against trivial evidences. In this note I point out that the number of remnants in our Universe could be finite, at least if the value of the cosmological constant is positive, as present observational data could indicate. Nevertheless, it is not clear if a huge but finite number of states is phenomenologically allowed.

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