Quantum critical magnetotransport at a continuous metal-insulator transition
Source abstract
Abstract
In contrast to the seminal weak localization prediction of a noncritical Hall constant (${R}H$) at the Anderson metal-insulator transition (MIT), ${R}H$ in quite a few real disordered systems exhibits both a strong $T$ dependence and critical scaling near their MIT. Here we investigate these issues in detail within a nonperturbative ``strong localization'' regime using cluster-dynamical mean-field theory (CDMFT). We uncover (i) clear and unconventional quantum-critical scaling of the Gell-Mann law, or $\ensuremath{\gamma}$ function for magnetotransport, finding that $\ensuremath{\gamma}({g}xy)=\frac{d[\text{log}({g}xy)]}{d[\text{log}(T)]}\ensuremath{\simeq}\phantom{\rule{4pt}{0ex}}\mathrm{log}({g}xy)$ over a wide range spanning the continuous MIT, very similar to that seen for the longitudinal conductivity, and (ii) strongly $T$ dependent and clear quantum critical scaling in both transverse conductivity and ${R}H$ at the MIT. We show that these surprising results are in comprehensive and very good accord with signatures of a novel Mott-like localization in NbN near the MIT, providing substantial support for our ``strong'' localization view.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Quantum and electron transport phenomena · Magnetic and transport properties of perovskites and related materials · Physics of Superconductivity and Magnetism
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (20)
Show source-provided references
1. D. Pines · 1999
2. 10.1103/RevModPhys.70.103910.1103/RevModPhys.70.1039 ↗
3. 10.1103/PhysRevLett.67.208810.1103/PhysRevLett.67.2088 ↗
4. 10.1038/nature0312910.1038/nature03129 ↗
5. 10.1103/RevModPhys.57.28710.1103/RevModPhys.57.287 ↗
6. 10.1103/PhysRevLett.55.52210.1103/PhysRevLett.55.522 ↗
7. 10.1103/PhysRevB.24.402510.1103/PhysRevB.24.4025 ↗
8. 10.1103/PhysRevB.80.13451410.1103/PhysRevB.80.134514 ↗
9. 10.1103/PhysRevB.22.514210.1103/PhysRevB.22.5142 ↗
10. 10.1126/science.111566010.1126/science.1115660 ↗
11. 10.1103/PhysRevB.94.08111510.1103/PhysRevB.94.081115 ↗
12. 10.1103/PhysRevB.80.08511710.1103/PhysRevB.80.085117 ↗
13. 10.1209/0295-5075/77/2700710.1209/0295-5075/77/27007 ↗
14. 10.1103/PhysRevB.95.12511610.1103/PhysRevB.95.125116 ↗
15. 10.1103/PhysRevB.55.390710.1103/PhysRevB.55.3907 ↗
16. 10.1103/PhysRevB.59.180010.1103/PhysRevB.59.1800 ↗
17. 10.1103/RevModPhys.75.133310.1103/RevModPhys.75.1333 ↗
18. 10.1103/PhysRev.109.149210.1103/PhysRev.109.1492 ↗
19. 10.1103/PhysRevLett.79.45510.1103/PhysRevLett.79.455 ↗
20. 10.1103/PhysRevLett.107.02640110.1103/PhysRevLett.107.026401 ↗