A paper written in 2020 by Harlow and Shaghoulian (reference 1) proposes a connection between unitary black hole evaporation and the non-existence of global symmetries in quantum gravity. In passing (page 6), they make this statement about a different connection, namely between locality and black hole remnants (which never evaporate):
...Einstein gravity is not renormalizable in $3+1$ dimensions..., and so far the “asymptotic safety” program that looks for a strongly-coupled UV fixed point for Einstein gravity in $3 + 1$ dimensions (such as the proponents of loop quantum gravity hope to find) has been unsuccessful. Moreover even if such a program were successful, the above examples suggest that it would lead to black holes whose entropy is not consistent with the Bekenstein-Hawking formula..., basically because locality would ensure the validity of UV/IR decoupling so one would be able to explicitly construct remnants. ...these remnants would necessarily involve high-energy degrees of freedom in some essential way.
Why would the "validity of UV/IR decoupling" allow us to explicitly construct remnants? Are they merely saying that such a theory would necessarily have remnants? That I could believe. But they seem to be saying that we would automatically be able to explicitly construct those remnants. Is that really what they mean? If so, then how does that follow from the validity of UV/IR decoupling?
- Harlow and Shaghoulian, Global symmetry, Euclidean gravity, and the black hole information problem (https://arxiv.org/abs/2010.10539)