Marginal deformations \& rotating horizons
From MaRDI portal
Publication:1707753
DOI10.1007/JHEP12(2017)095zbMATH Open1383.81175arXiv1707.03380WikidataQ112153931 ScholiaQ112153931MaRDI QIDQ1707753
Author name not available (Why is that?)
Publication date: 3 April 2018
Published in: (Search for Journal in Brave)
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.
Full work available at URL: https://arxiv.org/abs/1707.03380
No records found.
No records found.
This page was built for publication: Marginal deformations \& rotating horizons
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q1707753)