Complex biphase nature of the superconducting dome of the FeSe phase diagram
Source abstract
Abstract
Single crystal synchrotron x-ray diffraction as a function of temperature and pressure has revealed a complex biphase mixture in superconducting FeSe. Based on our experimental results, we construct a phase diagram where structural behavior and superconducting properties of FeSe are found to be correlated. We show that below 6 GPa, where pressure promotes the superconducting critical temperature, the FeSe structure is composed of two-dimensional layers of edge-shared $\mathrm{FeS}{\mathrm{e}}4$ tetrahedra, while above 6 GPa, the superconductivity is strongly suppressed on formation of a new orthorhombic polymorph characterized by a three-dimensional network of face sharing $\mathrm{FeS}{\mathrm{e}}6$ octahedra. Therefore, changes in topology and connectivity of the FeSe structure are found to be detrimental to superconductivity. The previously controversial crystal structure of the high-pressure polymorph of FeSe was unambiguously determined in the present paper. High-pressure FeSe adopts an orthorhombic MnP-type structure (Pnma) which corresponds to a slightly distorted hexagonal NiAs-type arrangement ($P{6}3/mmc$). The structural transformation from the low- to high-pressure FeSe polymorph is first order in nature and is manifested as antiparallel displacements within the Fe and Se sublattices.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Iron-based superconductors research · Rare-earth and actinide compounds · Corporate Taxation and Avoidance
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (42)
Show source-provided references
1. 10.1103/RevModPhys.84.138310.1103/RevModPhys.84.1383 ↗
2. 10.1038/2783810.1038/27838 ↗
3. 10.1103/RevModPhys.87.85510.1103/RevModPhys.87.855 ↗
4. 10.1088/1367-2630/11/2/02500910.1088/1367-2630/11/2/025009 ↗
5. 10.1021/ja800073m10.1021/ja800073m ↗
6. 10.1073/pnas.080732510510.1073/pnas.0807325105 ↗
7. 10.1103/PhysRevB.82.18052010.1103/PhysRevB.82.180520 ↗
8. 10.1088/0953-8984/23/5/05220310.1088/0953-8984/23/5/052203 ↗
9. 10.1103/PhysRevB.83.06051210.1103/PhysRevB.83.060512 ↗
10. 10.1088/0953-8984/28/29/29300210.1088/0953-8984/28/29/293002 ↗
11. 10.1038/nmat249110.1038/nmat2491 ↗
12. 10.1038/nmat364810.1038/nmat3648 ↗
13. 10.1038/nmat415310.1038/nmat4153 ↗
14. 10.1103/PhysRevLett.103.05700210.1103/PhysRevLett.103.057002 ↗
15. 10.1073/pnas.160656211310.1073/pnas.1606562113 ↗
16. 10.1103/PhysRevB.94.15513810.1103/PhysRevB.94.155138 ↗
17. 10.1103/PhysRevLett.104.08700310.1103/PhysRevLett.104.087003 ↗
18. 10.1103/PhysRevB.85.06451710.1103/PhysRevB.85.064517 ↗
19. 10.7566/JPSJ.84.06370110.7566/JPSJ.84.063701 ↗
20. 10.1038/ncomms1214610.1038/ncomms12146 ↗
21. 10.1038/ncomms1272810.1038/ncomms12728 ↗
22. 10.7566/JPSJ.83.01370210.7566/JPSJ.83.013702 ↗
23. 10.1103/PhysRevB.93.06450310.1103/PhysRevB.93.064503 ↗
24. 10.1063/1.300061610.1063/1.3000616 ↗
25. 10.1088/0953-8984/21/23/23220210.1088/0953-8984/21/23/232202 ↗
26. 10.1209/0295-5075/86/2700110.1209/0295-5075/86/27001 ↗
27. 10.1103/PhysRevB.80.06450610.1103/PhysRevB.80.064506 ↗
28. 10.1021/jp106044610.1021/jp1060446 ↗
29. 10.1088/0953-8984/23/20/20560110.1088/0953-8984/23/20/205601 ↗
30. 10.1088/0953-2048/28/10/10500910.1088/0953-2048/28/10/105009 ↗
31. 10.1103/PhysRevB.89.14410610.1103/PhysRevB.89.144106 ↗
32. 10.1063/1.132841010.1063/1.1328410 ↗
33. 10.1126/science.176.4032.28410.1126/science.176.4032.284 ↗
34. 10.1107/S205327331402637010.1107/S2053273314026370 ↗
35. 10.1103/PhysRevB.91.17451010.1103/PhysRevB.91.174510 ↗
36. 10.1016/j.ssc.2009.02.01110.1016/j.ssc.2009.02.011 ↗
37. 10.3891/acta.chem.scand.16-028710.3891/acta.chem.scand.16-0287 ↗
38. 10.1103/PhysRevB.10.124810.1103/PhysRevB.10.1248 ↗
39. P. Toledano · 199610.1142/2848 ↗
40. 10.1143/JPSJ.78.09370310.1143/JPSJ.78.093703 ↗
41. 10.1103/PhysRevB.81.20511910.1103/PhysRevB.81.205119 ↗
42. 10.1103/PhysRevLett.118.14700410.1103/PhysRevLett.118.147004 ↗