Soliton Stars as Holographic Confined Fermi Liquids
arXiv:1201.0764 · doi:10.1007/JHEP02(2012)137
Abstract
In this paper, we study a holographic dual of a confined fermi liquid state by putting a charged fluid of fermions in the AdS soliton geometry. This can be regarded as a confined analogue of electron stars. Depending on the parameters such as the mass and charge of the bulk fermion field, we found three different phase structures when we change the values of total charge density at zero temperature. In one of the three cases, our confined solution (called soliton star) is always stable and this solution approaches to the electron star away from the tip. In both the second and third case, we find a confinement/deconfinement phase transition. Moreover, in the third one, there is a strong indication that the soliton star decays into an inhomogeneous solution. We also analyze the probe fermion equations (in the WKB approximation) in the background of this soliton star geometry to confirm the presence of many fermi-surfaces in the system.
39 pages, 14 figures
References in corpus (8)
- Effective Holographic Theories for low-temperature condensed matter systems
- Hidden Fermi surfaces in compressible states of gauge-gravity duality
- Holographic Fermi Surfaces and Entanglement Entropy
- Holography of Dyonic Dilaton Black Branes
- Complete Phase Diagrams for a Holographic Superconductor/Insulator System
- Phase Diagram of N=4 Super-Yang-Mills Theory with R-Symmetry Chemical Potentials
- Degenerate Stars and Gravitational Collapse in AdS/CFT
- Electron star birth: A continuous phase transition at nonzero density