journal article·2017-10-10Open access

Quantum critical magnetotransport at a continuous metal-insulator transition

P. Haldar, M. S. Laad, S. R. Hassan, Madhavi Chand, Pratap Raychaudhuri

Physical Review B· Volume 96· Issue 15

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 ↗