journal article·2019-09-18

Superconductivity with strong electron-phonon coupling in noncentrosymmetric W3Al2C

T. P. Ying, Y. P. Qi, H. Hosono

Physical Review B· Volume 100· Issue 9
Publisher page

Abstract

We report the discovery of superconductivity in ${\mathrm{W}}3{\mathrm{Al}}2\mathrm{C}$ (${T}c=7.6\phantom{\rule{0.16em}{0ex}}\mathrm{K}$) synthesized by high-pressure method. ${\mathrm{W}}3{\mathrm{Al}}2\mathrm{C}$ is isostructural to ${\mathrm{Mo}}3{\mathrm{Al}}2\mathrm{C}$ (space group $P{4}132$) but with stronger spin-orbit coupling (SOC). Different from the ${\mathrm{Mo}}3{\mathrm{Al}}2\mathrm{C}$ with metallic nature, the resistivity of the normal state of ${\mathrm{W}}3{\mathrm{Al}}2\mathrm{C}$ shows a nonmetallic behavior. A specific-heat jump of $\mathrm{\ensuremath{\Delta}}{C}es/\ensuremath{\gamma}{T}c=2.7$ and gap energy of $2\mathrm{\ensuremath{\Delta}}(0)/\ensuremath{\gamma}{T}c=5.43$ are observed, which are much larger than that of ${\mathrm{Mo}}3{\mathrm{Al}}2\mathrm{C}$ (2.1 and 4.03) and the expectation of Bardeen-Cooper-Schrieffer theory (1.43 and 3.52). However, the Sommerfeld coefficient of ${\mathrm{W}}3{\mathrm{Al}}2\mathrm{C}$ is less than half of that of its Mo counterpart, and the specific heat above 2 K shows a power-law divergence following ${C}es/\ensuremath{\gamma}{T}c\phantom{\rule{4pt}{0ex}}\ensuremath{\sim}\phantom{\rule{4pt}{0ex}}{(T/{T}c)}3.3$ rather than an exponential relation. Theoretical calculations show that the Fermi surface of ${\mathrm{W}}3{\mathrm{Al}}2\mathrm{C}$ is dominated by W-$5d$ electrons and the inclusion of SOC significantly changes its band structure, density of states, and Fermi surface topology. The realization of superconductivity by replacing $4d$ Mo toward $5d\phantom{\rule{0.16em}{0ex}}\mathrm{W}$ provides a candidate for the search of potential triplet superconductors with enhanced SOC.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: MXene and MAX Phase Materials · Iron-based superconductors research · Superconductivity in MgB2 and Alloys

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

References (45)

Show source-provided references
1. 10.1103/PhysRevLett.92.02700310.1103/PhysRevLett.92.027003 ↗
2. 10.1103/PhysRevLett.87.03700410.1103/PhysRevLett.87.037004 ↗
3. 10.1103/PhysRevLett.99.25700410.1103/PhysRevLett.99.257004 ↗
4. 10.1143/JPSJ.76.07370810.1143/JPSJ.76.073708 ↗
5. 10.1103/PhysRevLett.102.11700710.1103/PhysRevLett.102.117007 ↗
6. 10.1103/PhysRevB.79.14450910.1103/PhysRevB.79.144509 ↗
7. 10.1103/PhysRevB.87.18050310.1103/PhysRevB.87.180503 ↗
8. 10.1103/PhysRevB.89.02451710.1103/PhysRevB.89.024517 ↗
9. 10.1103/PhysRevLett.112.10700210.1103/PhysRevLett.112.107002 ↗
10. 10.1103/PhysRevLett.115.26700110.1103/PhysRevLett.115.267001 ↗
11. 10.1103/PhysRevB.95.18451410.1103/PhysRevB.95.184514 ↗
12. 10.1126/sciadv.aao451310.1126/sciadv.aao4513 ↗
13. 10.1103/PhysRevLett.93.24700410.1103/PhysRevLett.93.247004 ↗
14. 10.1143/JPSJ.74.101410.1143/JPSJ.74.1014 ↗
15. 10.1103/PhysRevB.72.10450610.1103/PhysRevB.72.104506 ↗
16. 10.1103/PhysRevLett.97.01700610.1103/PhysRevLett.97.017006 ↗
17. 10.1103/PhysRevLett.98.04700210.1103/PhysRevLett.98.047002 ↗
18. 10.1088/0953-2048/23/10/10501810.1088/0953-2048/23/10/105018 ↗
19. 10.1088/1742-6596/400/2/02209610.1088/1742-6596/400/2/022096 ↗
20. 10.1103/PhysRevB.82.06451110.1103/PhysRevB.82.064511 ↗
21. 10.1103/PhysRevB.84.21250110.1103/PhysRevB.84.212501 ↗
22. 10.7566/JPSJ.82.07370910.7566/JPSJ.82.073709 ↗
23. 10.1103/PhysRevB.85.05250110.1103/PhysRevB.85.052501 ↗
24. 10.1103/PhysRevB.82.06451210.1103/PhysRevB.82.064512 ↗
25. 10.1103/PhysRevB.84.13450610.1103/PhysRevB.84.134506 ↗
26. 10.1103/PhysRevB.90.05452210.1103/PhysRevB.90.054522 ↗
27. 10.1016/0921-4526(93)90108-I10.1016/0921-4526(93)90108-I ↗
28. 10.1107/S002188981103897010.1107/S0021889811038970 ↗
29. 10.1103/PhysRevB.47.55810.1103/PhysRevB.47.558 ↗
30. 10.1016/0927-0256(96)00008-010.1016/0927-0256(96)00008-0 ↗
31. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
32. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
33. 10.1103/PhysRevB.13.518810.1103/PhysRevB.13.5188 ↗
34. 10.1103/PhysRevB.86.10410510.1103/PhysRevB.86.104105 ↗
35. 10.1103/PhysRevLett.109.21700210.1103/PhysRevLett.109.217002 ↗
36. 10.1126/sciadv.aar796910.1126/sciadv.aar7969 ↗
37. 10.7567/APEX.11.05310210.7567/APEX.11.053102 ↗
38. 10.1126/sciadv.150128310.1126/sciadv.1501283 ↗
39. 10.1126/science.aav864510.1126/science.aav8645 ↗
40. 10.7566/JPSJ.88.04370210.7566/JPSJ.88.043702 ↗
41. 10.1143/JPSJ.78.11500210.1143/JPSJ.78.115002 ↗
42. 10.1088/1361-6633/80/3/03650110.1088/1361-6633/80/3/036501 ↗
43. 10.1088/1361-648X/aac61d10.1088/1361-648X/aac61d ↗
44. 10.1103/PhysRevLett.95.24700410.1103/PhysRevLett.95.247004 ↗
45. 10.1143/JPSJ.75.04370310.1143/JPSJ.75.043703 ↗