Marginal Deformations and Rotating Horizons
Dionysios Anninos, Tarek Anous, and Raffaele Tito D'Agnolo

TL;DR
This paper investigates a disordered quantum system inspired by extremal black holes, revealing a phase transition influenced by marginal deformations and drawing parallels with rotating black hole horizons.
Contribution
It introduces a model with $SU(2)$ symmetry and marginal deformations, analyzing its phase transition and connecting it to black hole horizon phenomena.
Findings
Identifies a quantum phase transition at a critical marginal coupling.
Calculates critical exponents for the phase transition.
Draws parallels between quantum mechanics and black hole horizon behavior.
Abstract
Motivated by the near-horizon geometry of four-dimensional extremal black holes, we study a disordered quantum mechanical system invariant under a global symmetry. As in the Sachdev-Ye-Kitaev model, this system exhibits an approximate symmetry at low energies, but also allows for a continuous family of breaking marginal deformations. Beyond a certain critical value for the marginal coupling, the model exhibits a quantum phase transition from the gapless phase to a gapped one and we calculate the critical exponents of this transition. We also show that charged, rotating extremal black holes exhibit a transition when the angular velocity of the horizon is tuned to a certain critical value. Where possible we draw parallels between the disordered quantum mechanics and charged, rotating black holes.
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