journal article·2017-11-16Open access

Spin excitation anisotropy in the optimally isovalent-doped superconductor BaFe2(As0.7P0.3)2

Ding Hu, Wenliang Zhang, Yuan Wei, Bertrand Roessli, Markos Skoulatos, Louis Pierre Regnault, Genfu Chen, Yu Song, Huiqian Luo, Shiliang Li, Pengcheng Dai

Physical Review B· Volume 96· Issue 18

Abstract

We use neutron polarization analysis to study spin excitation anisotropy in the optimally isovalent-doped superconductor ${\mathrm{BaFe}}2$(${\mathrm{As}}0.7{\mathrm{P}}0.3$)${}2$ (${T}c=30$ K). Different from optimally hole- and electron-doped ${\mathrm{BaFe}}2{\mathrm{As}}2$, where there is a clear spin excitation anisotropy in the paramagnetic tetragonal state well above ${T}c$, we find no spin excitation anisotropy for energies above 2 meV in the normal state of ${\mathrm{BaFe}}2$(${\mathrm{As}}0.7{\mathrm{P}}0.3$)${}2$. Upon entering the superconducting state, significant spin excitation anisotropy develops at the antiferromagnetic (AF) zone center ${\mathbf{Q}}_{\mathrm{AF}}=(1,0,L=\mathrm{odd})$, while the magnetic spectrum is isotropic at the zone boundary $\mathbf{Q}=(1,0,L=\mathrm{even})$. By comparing the temperature, wave vector, and polarization dependence of the spin excitation anisotropy in ${\mathrm{BaFe}}2$(${\mathrm{As}}0.7{\mathrm{P}}0.3$)${}2$ and hole-doped ${\mathrm{Ba}}0.67{\mathrm{K}}0.33{\mathrm{Fe}}2{\mathrm{As}}2$ (${T}c=38$ K), we conclude that such anisotropy arises from spin-orbit coupling and is associated with the nearby AF order and superconductivity.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Iron-based superconductors research · Rare-earth and actinide compounds · Superconductivity in MgB2 and Alloys

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

References (53)

Show source-provided references
1. 10.1103/PhysRevLett.101.02640610.1103/PhysRevLett.101.026406 ↗
2. 10.1103/PhysRevLett.101.07640210.1103/PhysRevLett.101.076402 ↗
3. 10.1021/ja800073m10.1021/ja800073m ↗
4. 10.1038/nature0705710.1038/nature07057 ↗
5. 10.1080/00018732.2010.51348010.1080/00018732.2010.513480 ↗
6. 10.1103/RevModPhys.87.85510.1103/RevModPhys.87.855 ↗
7. 10.1038/nphys287710.1038/nphys2877 ↗
8. 10.1088/0034-4885/74/12/12450810.1088/0034-4885/74/12/124508 ↗
9. 10.1103/RevModPhys.84.138310.1103/RevModPhys.84.1383 ↗
10. 10.1038/natrevmats.2016.1710.1038/natrevmats.2016.17 ↗
11. 10.1103/PhysRevLett.104.15700110.1103/PhysRevLett.104.157001 ↗
12. 10.1126/science.aab010310.1126/science.aab0103 ↗
13. 10.1038/nphys359410.1038/nphys3594 ↗
14. 10.1103/PhysRevLett.114.16700110.1103/PhysRevLett.114.167001 ↗
15. 10.1103/PhysRevB.91.15510610.1103/PhysRevB.91.155106 ↗
16. 10.1103/PhysRevB.95.20510710.1103/PhysRevB.95.205107 ↗
17. 10.1103/PhysRevLett.118.08700310.1103/PhysRevLett.118.087003 ↗
18. 10.1103/PhysRevB.92.21450910.1103/PhysRevB.92.214509 ↗
19. 10.1103/PhysRevB.90.21451410.1103/PhysRevB.90.214514 ↗
20. 10.1007/s10948-013-2212-610.1007/s10948-013-2212-6 ↗
21. 10.1103/PhysRevB.85.05441110.1103/PhysRevB.85.054411 ↗
22. 10.1103/PhysRevB.83.14050610.1103/PhysRevB.83.140506 ↗
23. 10.1103/PhysRevB.82.06451510.1103/PhysRevB.82.064515 ↗
24. 10.1103/PhysRevB.86.06450310.1103/PhysRevB.86.064503 ↗
25. 10.1103/PhysRevLett.110.13700110.1103/PhysRevLett.110.137001 ↗
26. 10.1103/PhysRevLett.111.10700610.1103/PhysRevLett.111.107006 ↗
27. 10.1103/PhysRevB.90.14050210.1103/PhysRevB.90.140502 ↗
28. 10.1103/PhysRevB.86.06041010.1103/PhysRevB.86.060410 ↗
29. 10.1103/PhysRevX.3.04103610.1103/PhysRevX.3.041036 ↗
30. 10.1103/PhysRevB.87.08110110.1103/PhysRevB.87.081101 ↗
31. 10.1103/PhysRevB.90.10050210.1103/PhysRevB.90.100502 ↗
32. 10.1103/PhysRevB.94.21451610.1103/PhysRevB.94.214516 ↗
33. 10.1038/s41598-017-10208-110.1038/s41598-017-10208-1 ↗
34. 10.1103/PhysRevX.7.02102510.1103/PhysRevX.7.021025 ↗
35. 10.1103/PhysRevLett.101.10700610.1103/PhysRevLett.101.107006 ↗
36. 10.1038/ncomms484510.1038/ncomms4845 ↗
37. 10.1103/PhysRevB.91.06050510.1103/PhysRevB.91.060505 ↗
38. 10.1038/nphys362910.1038/nphys3629 ↗
39. 10.1103/PhysRevLett.101.11700410.1103/PhysRevLett.101.117004 ↗
40. 10.1088/1367-2630/11/2/02500810.1088/1367-2630/11/2/025008 ↗
41. 10.1103/PhysRevLett.106.25700110.1103/PhysRevLett.106.257001 ↗
42. 10.1103/PhysRevLett.110.25700110.1103/PhysRevLett.110.257001 ↗
43. 10.1088/0953-8984/21/38/38220310.1088/0953-8984/21/38/382203 ↗
44. 10.1146/annurev-conmatphys-031113-13392110.1146/annurev-conmatphys-031113-133921 ↗
45. 10.1103/PhysRevLett.114.15700210.1103/PhysRevLett.114.157002 ↗
46. 10.1038/nature0762510.1038/nature07625 ↗
47. 10.1103/PhysRevLett.102.10700510.1103/PhysRevLett.102.107005 ↗
48. 10.1103/PhysRevLett.102.10700610.1103/PhysRevLett.102.107006 ↗
49. 10.1038/ncomms387410.1038/ncomms3874 ↗
50. 10.1103/PhysRevLett.111.16700210.1103/PhysRevLett.111.167002 ↗
51. 10.1103/PhysRevB.94.09450410.1103/PhysRevB.94.094504 ↗
52. 10.1103/PhysRevB.86.09452110.1103/PhysRevB.86.094521 ↗
53. 10.1103/PhysRevB.96.02040410.1103/PhysRevB.96.020404 ↗