Fractionalization of holographic Fermi surfaces
Sean A. Hartnoll, Liza Huijse
TL;DR
The paper addresses how zero-temperature, finite-density phases in holographic theories organize when the bulk electric flux can be sourced by either bulk fermions, an extremal horizon, or both. By coupling a charged fluid of fermions to an Einstein-Maxwell-dilaton theory, they realize transitions between mesonic, fully fractionalized, and partially fractionalized phases, with the onset of fractionalization potentially continuous or first-order. A continuous transition is controlled by an emergent IR Lifshitz fixed point with dynamical exponent $z>1$, while complex scaling dimensions can preempt it with a first-order transition. The resulting phase diagram, parameterized by the UV dilaton coupling $\phi_0$ and chemical potential $\hat\mu$, exhibits Lifshitz-mediated crossovers and charge fractionation $\hat Q_{\text{frac.}}/\hat Q$, offering a concrete holographic platform for FL/FL$^*$/NFL-like behavior and the study of order parameters distinguishing fractionalized from mesonic phases.
Abstract
Zero temperature states of matter are holographically described by a spacetime with an asymptotic electric flux. This flux can be sourced either by explicit charged matter fields in the bulk, by an extremal black hole horizon, or by a combination of the two. We refer to these as mesonic, fully fractionalized and partially fractionalized phases of matter, respectively. By coupling a charged fluid of fermions to an asymptotically AdS_4 Einstein-Maxwell-dilaton theory, we exhibit quantum phase transitions between all three of these phases. The onset of fractionalization can be either a first order or continuous phase transition. In the latter case, at the quantum critical point the theory displays an emergent Lifshitz scaling symmetry in the IR.
