Universal fermionic spectral functions from string theory
Jerome P. Gauntlett, Julian Sonner, Daniel Waldram

TL;DR
This paper presents the first holographic calculation of a fermionic response in a strongly coupled 3D system with supergravity duals, revealing universal features like a phonino pole and spectral depletion without a Fermi surface.
Contribution
It provides a universal fermionic spectral function for 3D N=2 SCFTs with supergravity duals, highlighting novel low-frequency behavior and the absence of a Fermi surface.
Findings
Spectral function has a phonino pole.
No Fermi surface observed at finite charge density.
Spectral weight shows power-law depletion at low frequencies.
Abstract
We carry out the first holographic calculation of a fermionic response function for a strongly coupled system with an explicit D=10 or D=11 supergravity dual. By considering the supersymmetry current, we obtain a universal result applicable to all d=3 N=2 SCFTs with such duals. Surprisingly, the spectral function does not exhibit a Fermi surface, despite the fact that the system is at finite charge density. We show that it has a phonino pole and at low frequencies there is a depletion of spectral weight with a power-law scaling which is governed by a locally quantum critical point.
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