A universal formula for the density of states in theories with finite-group symmetry
Daniel Harlow, Hirosi Ooguri

TL;DR
This paper derives a universal formula for the density of black hole microstates transforming under finite-group symmetries using Euclidean gravity, providing a new proof of the completeness hypothesis and proposing broader applicability in quantum field theories.
Contribution
It introduces a universal formula for the density of states in theories with finite-group symmetry, linking gravity and quantum field theory insights.
Findings
Formula applies to black hole microstates in finite gauge groups
Provides proof of the completeness hypothesis for finite gauge fields
Suggests the formula's applicability to high-energy quantum field theories with finite symmetries
Abstract
In this paper we use Euclidean gravity to derive a simple formula for the density of black hole microstates which transform in each irreducible representation of any finite gauge group. Since each representation appears with nonzero density, this gives a new proof of the completeness hypothesis for finite gauge fields. Inspired by the generality of the argument we further propose that the formula applies at high energy in any quantum field theory with a finite-group global symmetry, and give some evidence for this conjecture.
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