Fermionic spectral functions in backreacting p-wave superconductors at finite temperature
DOI10.1007/JHEP04(2017)087zbMath1378.81118arXiv1610.04268OpenAlexW2538524426MaRDI QIDQ1691528
Nicolas Esteban Grandi, Adrián R. Lugo, Gastón L. Giordano
Publication date: 23 January 2018
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1610.04268
AdS/CFT correspondenceblack holesgauge-gravity correspondenceholography and condensed matter physics (AdS/CMT)
Two-dimensional field theories, conformal field theories, etc. in quantum mechanics (81T40) Black holes (83C57) Classical and relativistic thermodynamics (80A10) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (1)
Cites Work
- Unnamed Item
- Linear resistivity from non-abelian black holes
- Photoemission ``experiments on holographic superconductors
- Holographic phase transition from dyons in an AdS black hole background
- Fermion correlators in non-abelian holographic superconductors
- Holography and AdSs\({}_{4}\) self-gravitating dyons
- Gauge theory correlators from non-critical string theory
- Degenerate stars and gravitational collapse in ads/CFT
- Holographic superconductors
- Anti de Sitter space and holography
- The large-\(N\) limit of superconformal field theories and supergravity
- Normalizable fermion modes in a holographic superconductor
- Fermionic operator mixing in holographic p-wave superfluids
- Holographic phase transitions from higgsed, non abelian charged black holes
- Holographic non-Fermi-liquid fixed points
- String Theory, Quantum Phase Transitions, and the Emergent Fermi Liquid
- Real‐time response in AdS/CFT with application to spinors
- Lectures on holographic methods for condensed matter physics
- Building a Holographic Superconductor
- Phase transitions near black hole horizons
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