Beyond universal behavior in the one-dimensional chain with random nearest-neighbor hopping
Source abstract
Abstract
We study the one-dimensional nearest-neighbor tight-binding model of electrons with independently distributed random hopping and no on-site potential (i.e., off-diagonal disorder with particle-hole symmetry, leading to sublattice symmetry, for each realization). For nonsingular distributions of the hopping, it is known that the model exhibits a universal, singular behavior of the density of states $\ensuremath{\rho}(E)\ensuremath{\sim}1/|E{ln}3|E||$ and of the localization length $\ensuremath{\xi}(E)\ensuremath{\sim}|ln|E||$, near the band center $E=0$. (This singular behavior is also applicable to random XY and Heisenberg spin chains; it was first obtained by Dyson for a specific random harmonic oscillator chain.) Simultaneously, the state at $E=0$ shows a universal, subexponential decay at large distances $\ensuremath{\sim}exp[\ensuremath{-}\sqrt{r/{r}0}]$. In this study, we consider singular, but normalizable, distributions of hopping, whose behavior at small $t$ is of the form $\ensuremath{\sim}1/[t{ln}^{\ensuremath{\lambda}+1}(1/t)]$, characterized by a single, continuously tunable parameter $\ensuremath{\lambda}>0$. We find, using a combination of analytic and numerical methods, that while the universal result applies for $\ensuremath{\lambda}>2$, it no longer holds in the interval $0<\ensuremath{\lambda}<2$. In particular, we find that the form of the density of states singularity is enhanced (relative to the Dyson result) in a continuous manner depending on the nonuniversal parameter $\ensuremath{\lambda}$; simultaneously, the localization length shows a less divergent form at low energies and ceases to diverge below $\ensuremath{\lambda}=1$. For $\ensuremath{\lambda}<2$, the fall-off of the $E=0$ state at large distances also deviates from the universal result and is of the form $\ensuremath{\sim}exp[\ensuremath{-}{(r/{r}0)}^{1/\ensuremath{\lambda}}]$, which decays faster than an exponential for $\ensuremath{\lambda}<1$.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Quantum and electron transport phenomena · Quantum many-body systems · Physics of Superconductivity and Magnetism
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (72)
Show source-provided references
1. 10.1080/0001873610010127110.1080/00018736100101271 ↗
2. 10.1103/PhysRevLett.42.67310.1103/PhysRevLett.42.673 ↗
3. 10.1103/RevModPhys.57.28710.1103/RevModPhys.57.287 ↗
4. 10.1103/RevModPhys.80.135510.1103/RevModPhys.80.1355 ↗
5. 10.1103/PhysRev.109.149210.1103/PhysRev.109.1492 ↗
6. 10.1103/PhysRevLett.65.8810.1103/PhysRevLett.65.88 ↗
7. 10.1103/PhysRevLett.81.373510.1103/PhysRevLett.81.3735 ↗
8. 10.1103/PhysRevLett.82.406210.1103/PhysRevLett.82.4062 ↗
9. 10.1016/S0378-4371(98)00632-310.1016/S0378-4371(98)00632-3 ↗
10. 10.1103/PhysRevB.68.04510110.1103/PhysRevB.68.045101 ↗
11. 10.1103/PhysRevB.97.17420510.1103/PhysRevB.97.174205 ↗
12. 10.1103/PhysRev.92.133110.1103/PhysRev.92.1331 ↗
13. 10.1088/0022-3719/3/7/00110.1088/0022-3719/3/7/001 ↗
14. 10.1016/0003-4916(61)90115-410.1016/0003-4916(61)90115-4 ↗
15. 10.1103/PhysRevB.13.459710.1103/PhysRevB.13.4597 ↗
16. 10.1103/PhysRevB.18.56910.1103/PhysRevB.18.569 ↗
17. 10.1016/0378-4371(80)90142-910.1016/0378-4371(80)90142-9 ↗
18. 10.1088/0022-3719/10/6/00310.1088/0022-3719/10/6/003 ↗
19. 10.1103/PhysRevB.24.569810.1103/PhysRevB.24.5698 ↗
20. 10.1103/PhysRevB.24.359210.1103/PhysRevB.24.3592 ↗
21. 10.1103/PhysRevLett.49.33710.1103/PhysRevLett.49.337 ↗
22. 10.1088/0022-3719/19/22/01510.1088/0022-3719/19/22/015 ↗
23. 10.1007/BF0156061410.1007/BF01560614 ↗
24. 10.1007/BF0131215010.1007/BF01312150 ↗
25. 10.1103/PhysRevB.38.294810.1103/PhysRevB.38.2948 ↗
26. 10.1103/PhysRevB.49.319010.1103/PhysRevB.49.3190 ↗
27. 10.1103/PhysRevB.24.24410.1103/PhysRevB.24.244 ↗
28. 10.1103/PhysRevB.29.606310.1103/PhysRevB.29.6063 ↗
29. 10.1103/PhysRevB.34.38710.1103/PhysRevB.34.387 ↗
30. 10.1103/PhysRevLett.61.59710.1103/PhysRevLett.61.597 ↗
31. L. Bulaevskii · Sov. Phys. JETP · 1972 · 35 · 384
32. 10.1103/PhysRevB.23.584610.1103/PhysRevB.23.5846 ↗
33. 10.1103/PhysRevB.22.130510.1103/PhysRevB.22.1305 ↗
34. 10.1103/PhysRevLett.48.34410.1103/PhysRevLett.48.344 ↗
35. 10.1103/PhysRevLett.69.53410.1103/PhysRevLett.69.534 ↗
36. 10.1103/PhysRevB.50.379910.1103/PhysRevB.50.3799 ↗
37. 10.1103/PhysRevB.51.641110.1103/PhysRevB.51.6411 ↗
38. 10.1103/PhysRevLett.77.480410.1103/PhysRevLett.77.4804 ↗
39. 10.1103/PhysRevLett.78.247310.1103/PhysRevLett.78.2473 ↗
40. 10.1103/PhysRevB.59.1130810.1103/PhysRevB.59.11308 ↗
41. 10.1103/PhysRevLett.86.134310.1103/PhysRevLett.86.1343 ↗
42. 10.1103/PhysRevB.73.22420610.1103/PhysRevB.73.224206 ↗
43. 10.1103/PhysRevLett.84.291310.1103/PhysRevLett.84.2913 ↗
44. 10.1103/PhysRevB.64.11310710.1103/PhysRevB.64.113107 ↗
45. 10.1103/PhysRevB.67.06420210.1103/PhysRevB.67.064202 ↗
46. 10.1103/PhysRevB.90.20540410.1103/PhysRevB.90.205404 ↗
47. 10.1103/PhysRevB.66.01420410.1103/PhysRevB.66.014204 ↗
48. 10.1103/PhysRevB.71.24512410.1103/PhysRevB.71.245124 ↗
49. 10.1103/PhysRevB.70.19532910.1103/PhysRevB.70.195329 ↗
50. 10.1103/PhysRevB.90.12514110.1103/PhysRevB.90.125141 ↗
51. 10.1103/PhysRevB.92.21420510.1103/PhysRevB.92.214205 ↗
52. 10.1103/PhysRevB.94.14420210.1103/PhysRevB.94.144202 ↗
53. 10.1103/PhysRevB.97.01420610.1103/PhysRevB.97.014206 ↗
54. 10.1103/RevModPhys.88.03500510.1103/RevModPhys.88.035005 ↗
55. 10.1103/PhysRevB.63.22420410.1103/PhysRevB.63.224204 ↗
56. 10.1016/S0370-1573(00)00070-310.1016/S0370-1573(00)00070-3 ↗
57. 10.1103/RevModPhys.87.48310.1103/RevModPhys.87.483 ↗
58. 10.1103/PhysRevB.90.06020510.1103/PhysRevB.90.060205 ↗
59. 10.1088/0034-4885/56/12/00110.1088/0034-4885/56/12/001 ↗
60. B. V. Gnedenko · 1968
61. 10.7566/JPSJ.87.04300310.7566/JPSJ.87.043003 ↗
62. 10.1103/PhysRev.105.42510.1103/PhysRev.105.425 ↗
63. 10.1214/ss/117701065610.1214/ss/1177010656 ↗
64. R. Klages · 200810.1002/9783527622979 ↗
65. V. Balakrishnan · 2008
66. 10.1103/PhysRevLett.99.16060210.1103/PhysRevLett.99.160602 ↗
67. 10.1103/PhysRevE.95.05210210.1103/PhysRevE.95.052102 ↗
68. 10.1088/1742-5468/ab498810.1088/1742-5468/ab4988 ↗
69. 10.1088/1367-2630/ab41bb10.1088/1367-2630/ab41bb ↗
70. 10.1088/0022-3719/5/1/01010.1088/0022-3719/5/1/010 ↗
71. 10.1103/PhysRev.34.5710.1103/PhysRev.34.57 ↗
72. 10.1088/0953-8984/2/13/00510.1088/0953-8984/2/13/005 ↗