Detailed optical spectroscopy of hybridization gap and hidden-order transition in high-qualityURu2Si2single crystals
Source abstract
Abstract
We present a detailed temperature and frequency dependence of the optical conductivity measured on clean high-quality single crystals of ${\mathrm{URu}}2{\mathrm{Si}}2$ of $ac\text{\ensuremath{-}}$ and $ab\text{-plane}$ surfaces. Our data demonstrate the itinerant character of the narrow $5f$ bands, becoming progressively coherent as the temperature is lowered below a crossover temperature ${T}*\ensuremath{\sim}75$ K. ${T}*$ is higher than in previous reports as a result of a different sample preparation, which minimizes residual strain. We furthermore present the density-response (energy-loss) function of this compound, and determine the energies of the heavy-fermion plasmons with $a\text{\ensuremath{-}}$ and $c\text{-axis}$ polarization. Our observation of a suppression of optical conductivity below 50 meV along both the $a$ and $c$ axes, along with a heavy-fermion plasmon at 18 meV, points toward the emergence of a band of coherent charge carriers crossing the Fermi energy and the emergence of a hybridization gap on part of the Fermi surface. The evolution towards coherent itinerant states is accelerated below the hidden order temperature ${T}_{\mathrm{HO}}=17.5$ K. In the hidden order phase the low-frequency optical conductivity shows a single gap at $\ensuremath{\sim}6.5$ meV, which closes at ${T}_{\mathrm{HO}}$.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Rare-earth and actinide compounds · High-pressure geophysics and materials · Advanced Condensed Matter Physics
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (55)
Show source-provided references
1. 10.1103/PhysRevLett.55.272710.1103/PhysRevLett.55.2727 ↗
2. 10.1103/PhysRevLett.56.18510.1103/PhysRevLett.56.185 ↗
3. 10.1103/PhysRevLett.91.25640110.1103/PhysRevLett.91.256401 ↗
4. 10.1103/PhysRevB.78.01250410.1103/PhysRevB.78.012504 ↗
5. 10.1103/PhysRevB.77.11511710.1103/PhysRevB.77.115117 ↗
6. 10.1103/RevModPhys.83.130110.1103/RevModPhys.83.1301 ↗
7. 10.1080/14786435.2014.91642810.1080/14786435.2014.916428 ↗
8. 10.1103/PhysRevB.82.20510310.1103/PhysRevB.82.205103 ↗
9. 10.1103/PhysRevB.84.24110210.1103/PhysRevB.84.241102 ↗
10. 10.1007/BF0132342710.1007/BF01323427 ↗
11. 10.1103/PhysRevLett.61.130510.1103/PhysRevLett.61.1305 ↗
12. 10.1209/0295-5075/32/4/01410.1209/0295-5075/32/4/014 ↗
13. 10.1007/s00257005030010.1007/s002570050300 ↗
14. 10.1103/PhysRevB.86.03513210.1103/PhysRevB.86.035132 ↗
15. 10.1073/pnas.120824910910.1073/pnas.1208249109 ↗
16. 10.1103/PhysRevB.85.19510510.1103/PhysRevB.85.195105 ↗
17. 10.1103/PhysRevB.92.04512910.1103/PhysRevB.92.045129 ↗
18. 10.1103/PhysRevLett.113.26640510.1103/PhysRevLett.113.266405 ↗
19. 10.1126/science.125972910.1126/science.1259729 ↗
20. 10.1038/nature0907310.1038/nature09073 ↗
21. 10.1073/pnas.100589210710.1073/pnas.1005892107 ↗
22. 10.1103/PhysRevB.46.582610.1103/PhysRevB.46.5826 ↗
23. 10.1103/PhysRevB.55.1431810.1103/PhysRevB.55.14318 ↗
24. 10.1103/PhysRevLett.108.24640310.1103/PhysRevLett.108.246403 ↗
25. 10.1038/ncomms518810.1038/ncomms5188 ↗
26. 10.1038/nphys139210.1038/nphys1392 ↗
27. 10.1126/science.119735810.1126/science.1197358 ↗
28. 10.1103/PhysRevLett.86.68410.1103/PhysRevLett.86.684 ↗
29. 10.1103/PhysRevB.33.652710.1103/PhysRevB.33.6527 ↗
30. 10.1103/PhysRevB.84.18442010.1103/PhysRevB.84.184420 ↗
31. 10.1016/j.jmmm.2006.10.00810.1016/j.jmmm.2006.10.008 ↗
32. 10.1103/PhysRevLett.104.10640610.1103/PhysRevLett.104.106406 ↗
33. 10.1103/PhysRevB.91.03512910.1103/PhysRevB.91.035129 ↗
34. 10.1073/pnas.121884611010.1073/pnas.1218846110 ↗
35. 10.1103/RevModPhys.56.75510.1103/RevModPhys.56.755 ↗
36. 10.1103/RevModPhys.83.47110.1103/RevModPhys.83.471 ↗
37. G. D. Mahan · 200010.1007/978-1-4757-5714-9 ↗
38. 10.1103/PhysRevB.6.122610.1103/PhysRevB.6.1226 ↗
39. 10.1103/PhysRevB.84.16110110.1103/PhysRevB.84.161101 ↗
40. 10.1080/14786435.2014.90961310.1080/14786435.2014.909613 ↗
41. 10.1103/PhysRevLett.110.15640410.1103/PhysRevLett.110.156404 ↗
42. 10.1103/PhysRevLett.105.21640910.1103/PhysRevLett.105.216409 ↗
43. 10.1038/nphys136110.1038/nphys1361 ↗
44. 10.1103/PhysRevB.82.20510810.1103/PhysRevB.82.205108 ↗
45. 10.1103/PhysRevLett.111.12700210.1103/PhysRevLett.111.127002 ↗
46. 10.1103/PhysRevLett.110.18640110.1103/PhysRevLett.110.186401 ↗
47. 10.1103/PhysRevLett.58.146710.1103/PhysRevLett.58.1467 ↗
48. 10.1103/PhysRevLett.87.08720310.1103/PhysRevLett.87.087203 ↗
49. 10.1016/S0921-4526(01)01343-610.1016/S0921-4526(01)01343-6 ↗
50. 10.1103/PhysRevB.72.21441910.1103/PhysRevB.72.214419 ↗
51. 10.1103/PhysRevB.43.1280910.1103/PhysRevB.43.12809 ↗
52. 10.1038/nphys52210.1038/nphys522 ↗
53. 10.1088/0953-8984/21/19/19220210.1088/0953-8984/21/19/192202 ↗
54. 10.1143/JPSJ.79.06471910.1143/JPSJ.79.064719 ↗
55. 10.1038/ncomms532610.1038/ncomms5326 ↗