journal article·2021-11-08Open access

Strongly coupled phonon fluid and Goldstone modes in an anharmonic quantum solid: Transport and chaos

Evyatar Tulipman, Erez Berg

Physical Review B· Volume 104· Issue 19

Abstract

We study properties of thermal transport and quantum many-body chaos in a lattice model with $N\ensuremath{\rightarrow}\ensuremath{\infty}$ oscillators per site, coupled by strong anharmonic terms. We first consider a model with only optical phonons. We find that the thermal diffusivity ${D}_{\mathrm{th}}$ and chaos diffusivity ${D}L$ (defined as ${D}L={v}B2/{\ensuremath{\lambda}}L$, where ${v}B$ and ${\ensuremath{\lambda}}L$ are the butterfly velocity and the scrambling rate, respectively) satisfy ${D}_{\mathrm{th}}\ensuremath{\approx}\ensuremath{\gamma}{D}L$ with $\ensuremath{\gamma}\ensuremath{\gtrsim}1$. At intermediate temperatures, the model exhibits a quantum ``phonon fluid'' regime, where both diffusivities satisfy ${D}^{\ensuremath{-}1}\ensuremath{\propto}T$, and the thermal relaxation time and inverse scrambling rate are of the order the of Planckian timescale $\ensuremath{\hbar}/{k}BT$. We then introduce acoustic phonons to the model and study their effect on transport and chaos. The long-wavelength acoustic modes remain long-lived even when the system is strongly coupled, due to Goldstone's theorem. As a result, for $d=1,2$, we find that ${D}_{\mathrm{th}}/{D}L\ensuremath{\rightarrow}\ensuremath{\infty}$, while for $d=3, {D}_{\mathrm{th}}$ and ${D}L$ remain comparable.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Quantum, superfluid, helium dynamics · Thermal properties of materials · Quantum and electron transport phenomena

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

References (67)

Show source-provided references
1. 10.1103/PhysRevB.56.871410.1103/PhysRevB.56.8714 ↗
2. 10.1038/430512a10.1038/430512a ↗
3. S. Sachdev · 201110.1017/CBO9780511973765 ↗
4. 10.21468/SciPostPhys.6.5.06110.21468/SciPostPhys.6.5.061 ↗
5. 10.1126/science.122761210.1126/science.1227612 ↗
6. 10.1038/s41567-018-0334-210.1038/s41567-018-0334-2 ↗
7. 10.1038/s41567-019-0596-310.1038/s41567-019-0596-3 ↗
8. 10.1103/PhysRevLett.124.07680110.1103/PhysRevLett.124.076801 ↗
9. 10.1038/s41586-019-0923-y10.1038/s41586-019-0923-y ↗
10. 10.1038/s41586-021-03697-810.1038/s41586-021-03697-8 ↗
11. 10.1103/PhysRevLett.94.11160110.1103/PhysRevLett.94.111601 ↗
12. 10.1007/JHEP03(2014)06710.1007/JHEP03(2014)067 ↗
13. 10.1007/JHEP03(2015)05110.1007/JHEP03(2015)051 ↗
14. 10.1103/PhysRevB.89.24511610.1103/PhysRevB.89.245116 ↗
15. J. Zaanen · 201510.1017/CBO9781139942492 ↗
16. 10.1103/PhysRevB.95.15513110.1103/PhysRevB.95.155131 ↗
17. S. A. Hartnoll · 2018
18. 10.1103/PhysRevLett.119.21660110.1103/PhysRevLett.119.216601 ↗
19. 10.1103/PhysRevX.8.02104910.1103/PhysRevX.8.021049 ↗
20. 10.1103/PhysRevX.8.03102410.1103/PhysRevX.8.031024 ↗
21. 10.1103/PhysRevLett.123.06660110.1103/PhysRevLett.123.066601 ↗
22. A. Larkin · Sov. Phys. JETP · 1969 · 28 · 1200
23. 10.1007/JHEP08(2016)10610.1007/JHEP08(2016)106 ↗
24. 10.1103/PhysRevLett.117.09160110.1103/PhysRevLett.117.091601 ↗
25. 10.1038/nphys317410.1038/nphys3174 ↗
26. 10.1073/pnas.161818511410.1073/pnas.1618185114 ↗
27. 10.1103/PhysRevX.7.03104710.1103/PhysRevX.7.031047 ↗
28. 10.1007/JHEP10(2016)14310.1007/JHEP10(2016)143 ↗
29. 10.1007/JHEP06(2017)03010.1007/JHEP06(2017)030 ↗
30. 10.21468/SciPostPhys.2.3.01810.21468/SciPostPhys.2.3.018 ↗
31. 10.1103/PhysRevB.100.04514010.1103/PhysRevB.100.045140 ↗
32. 10.1007/JHEP05(2017)12510.1007/JHEP05(2017)125 ↗
33. 10.1103/PhysRevD.96.10600810.1103/PhysRevD.96.106008 ↗
34. 10.1103/PhysRevD.100.04601210.1103/PhysRevD.100.046012 ↗
35. 10.1007/JHEP01(2018)14010.1007/JHEP01(2018)140 ↗
36. 10.1073/pnas.170341611410.1073/pnas.1703416114 ↗
37. 10.1103/PhysRevLett.120.12590110.1103/PhysRevLett.120.125901 ↗
38. 10.1088/1361-648X/ab2db610.1088/1361-648X/ab2db6 ↗
39. 10.1073/pnas.191013111610.1073/pnas.1910131116 ↗
40. 10.1103/PhysRevB.104.03520810.1103/PhysRevB.104.035208 ↗
41. 10.1103/PhysRevResearch.2.03343110.1103/PhysRevResearch.2.033431 ↗
42. 10.1103/PhysRevLett.70.333910.1103/PhysRevLett.70.3339 ↗
43. 10.1103/PhysRevD.94.10600210.1103/PhysRevD.94.106002 ↗
44. 10.1103/PhysRevB.64.01440310.1103/PhysRevB.64.014403 ↗
45. 10.1103/PhysRevD.96.10601410.1103/PhysRevD.96.106014 ↗
46. 10.1007/JHEP04(2021)19710.1007/JHEP04(2021)197 ↗
47. 10.1007/JHEP10(2018)12710.1007/JHEP10(2018)127 ↗
48. 10.21468/SciPostPhys.9.1.00710.21468/SciPostPhys.9.1.007 ↗
49. 10.1007/JHEP05(2021)01410.1007/JHEP05(2021)014 ↗
50. J. M. Ziman · 1960
51. 10.1103/PhysRevLett.84.285710.1103/PhysRevLett.84.2857 ↗
52. 10.1103/RevModPhys.90.04100210.1103/RevModPhys.90.041002 ↗
53. M. Mezard · 198610.1142/0271 ↗
54. 10.1103/PhysRevB.103.18430510.1103/PhysRevB.103.184305 ↗
55. 10.1103/PhysRevB.98.20512410.1103/PhysRevB.98.205124 ↗
56. 10.1103/PhysRevE.99.01220610.1103/PhysRevE.99.012206 ↗
57. 10.1007/JHEP07(2019)10710.1007/JHEP07(2019)107 ↗
58. 10.1103/PhysRevLett.126.03060210.1103/PhysRevLett.126.030602 ↗
59. 10.1103/PhysRevD.96.06500510.1103/PhysRevD.96.065005 ↗
60. 10.1016/j.aop.2016.09.00610.1016/j.aop.2016.09.006 ↗
61. 10.1007/JHEP05(2015)13210.1007/JHEP05(2015)132 ↗
62. 10.1103/PhysRevB.95.13430210.1103/PhysRevB.95.134302 ↗
63. 10.1103/PhysRevB.100.23510410.1103/PhysRevB.100.235104 ↗
64. R. P. Feynman · 1965
65. G. D. Mahan · 200010.1007/978-1-4757-5714-9 ↗
66. 10.1103/PhysRevX.8.03106410.1103/PhysRevX.8.031064 ↗
67. A. Kamenev · 201110.1017/CBO9781139003667 ↗