Holographic metals at finite volume
Lucas Acito, Nicolas Grandi
TL;DR
This work analyzes a holographic metal at finite volume by constructing an electron star in asymptotically global AdS and examining its thermodynamic stability relative to RN-AdS black holes and Thermal AdS. Using a charged perfect fluid with Thomas–Fermi thermodynamics and a grand canonical ensemble, the authors map a phase diagram in the boundary variables $(T_ty, μ_ty)$, identifying a finite stable region for the electron star and a distinct first-order star–BH transition, with a zero-temperature quantum critical point at $μ_ty\approx1.435$ that organizes the phases. The zero-temperature analysis reveals a transition from TAdS$_4$ to Electron Star at $μ_ty=1$, and the overall phase structure is reminiscent of Hawking-Page physics but enriched by the star solution. These results provide a controlled platform to study finite-volume holographic metals and quantum criticality, with potential extensions to boundary correlators and holographic superconductivity on this background.
Abstract
We construct the electron star solution in asymptotically global AdS spacetime, and investigate its stability properties, both locally under perturbations and globally with respect to the Reissner-Nordström black hole and thermal AdS metrics. We interpret the resulting phase diagram as that of a holographic metal confined to a finite volume. We identify a quantum critical point at finite chemical potential, around which the different phases are organized.
