Extremal black hole decay in de Sitter space

Abstract

Abstract The decay of extremal charged black holes has been a useful guidance to derive consistency conditions in quantum gravity. In de Sitter space it has been argued that requiring (extremal) charged Nariai black holes to decay without forming a big crunch singularity yields the Festina Lente (FL) bound: particles with mass m s and charge q should satisfy m s 2 ≫ M p Hq $$ {m}_s^2\gg {M}_p Hq $$ , where M p is the Planck mass and H the Hubble parameter. Using a tunneling approach we show that the decay probability of charged black holes in de Sitter space in the s-wave sector is P ∼ exp(∆S b ), where ∆S b is the change in the black hole entropy. We find that the FL bound corresponds to ∆S b ≤ – 1 in the Nariai and probe limit. However, taking into account backreaction we identify unsuppressed decay channels, which might be subdominant, that violate this bound but nonetheless do not result in a big crunch for every observer.

Keywords

• Black Holes
• de Sitter space