journal article·2017-05-30Open access

Pair-checkerboard antiferromagnetic order in β−Fe4Se5 with 5×5 -ordered Fe vacancies

Miao Gao, Xin Kong, Xun-Wang Yan, Zhong-Yi Lu, Tao Xiang

Physical Review B· Volume 95· Issue 17

Abstract

The electronic structure of recently discovered $\ensuremath{\beta}\text{\ensuremath{-}}{\mathrm{Fe}}4{\mathrm{Se}}5$ with $\sqrt{5}\ifmmode\times\else\texttimes\fi{}\sqrt{5}$ ordered Fe vacancies is calculated using first-principles density functional theory. We find that the ground state is an antiferromagnetic (AFM) insulator in agreement with the experimental observation. In ${\mathrm{K}}2{\mathrm{Fe}}4{\mathrm{Se}}5$, it is known that the ground state is $\sqrt{5}\ifmmode\times\else\texttimes\fi{}\sqrt{5}$-blocked-checkerboard AFM ordered. But for this material, we find that the ground state is $\sqrt{5}\ifmmode\times\else\texttimes\fi{}\sqrt{5}$-pair-checkerboard AFM ordered, in which the intrablock four Fe spins exhibit the collinear AFM order and the interblock spins on any two nearest-neighboring sites are antiparallel aligned. This state is about 130 meV/Fe lower in energy than the $\sqrt{5}\ifmmode\times\else\texttimes\fi{}\sqrt{5}$-blocked-checkerboard AFM one. Electron doping can lower the energy of the $\sqrt{5}\ifmmode\times\else\texttimes\fi{}\sqrt{5}$-blocked-checkerboard AFM state and introduce a transition between these two states, suggesting that there is strong AFM fluctuation in FeSe-based materials upon doping. This provides a unified picture to understand the AFM orders in $\ensuremath{\beta}\text{\ensuremath{-}}{\mathrm{Fe}}4{\mathrm{Se}}5$ and in alkali-metal intercalated FeSe materials.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Iron-based superconductors research · Rare-earth and actinide compounds · Crystal Structures and Properties

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

References (36)

Show source-provided references
1. 10.1021/ja800073m10.1021/ja800073m ↗
2. 10.1038/nmat231510.1038/nmat2315 ↗
3. 10.1103/PhysRevB.81.20511910.1103/PhysRevB.81.205119 ↗
4. 10.1088/0953-2048/23/5/05401310.1088/0953-2048/23/5/054013 ↗
5. 10.1073/pnas.080732510510.1073/pnas.0807325105 ↗
6. 10.1103/PhysRevB.82.18052010.1103/PhysRevB.82.180520 ↗
7. 10.1088/0953-8984/23/5/05220310.1088/0953-8984/23/5/052203 ↗
8. 10.1209/0295-5075/94/2700910.1209/0295-5075/94/27009 ↗
9. 10.1209/0295-5075/93/4700410.1209/0295-5075/93/47004 ↗
10. 10.1038/nature1081310.1038/nature10813 ↗
11. 10.1038/srep0042610.1038/srep00426 ↗
12. 10.1103/PhysRevLett.106.08700510.1103/PhysRevLett.106.087005 ↗
13. 10.1103/PhysRevB.83.23320510.1103/PhysRevB.83.233205 ↗
14. 10.1088/0256-307X/28/8/08610410.1088/0256-307X/28/8/086104 ↗
15. 10.1103/PhysRevLett.109.26700310.1103/PhysRevLett.109.267003 ↗
16. 10.1103/PhysRevX.1.02102010.1103/PhysRevX.1.021020 ↗
17. 10.1038/ncomms291310.1038/ncomms2913 ↗
18. 10.1088/0953-8984/24/43/43570110.1088/0953-8984/24/43/435701 ↗
19. 10.1103/PhysRevB.84.06051110.1103/PhysRevB.84.060511 ↗
20. 10.1103/PhysRevB.91.02050310.1103/PhysRevB.91.020503 ↗
21. 10.1103/PhysRevB.83.14050510.1103/PhysRevB.83.140505 ↗
22. 10.1103/PhysRevLett.109.05700310.1103/PhysRevLett.109.057003 ↗
23. 10.1103/PhysRevB.84.05250210.1103/PhysRevB.84.052502 ↗
24. 10.1073/pnas.132116011110.1073/pnas.1321160111 ↗
25. 10.1103/PhysRevB.93.18450310.1103/PhysRevB.93.184503 ↗
26. 10.1088/0953-8984/21/39/39550210.1088/0953-8984/21/39/395502 ↗
27. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
28. 10.1103/PhysRevB.41.789210.1103/PhysRevB.41.7892 ↗
29. 10.1016/0304-8853(86)90900-510.1016/0304-8853(86)90900-5 ↗
30. 10.1103/PhysRevB.91.02050410.1103/PhysRevB.91.020504 ↗
31. 10.1038/nature0705710.1038/nature07057 ↗
32. 10.1103/PhysRevB.78.02050310.1103/PhysRevB.78.020503 ↗
33. 10.1103/PhysRevLett.103.05700210.1103/PhysRevLett.103.057002 ↗
34. 10.1103/PhysRevLett.102.17700310.1103/PhysRevLett.102.177003 ↗
35. 10.1002/jcc.2049510.1002/jcc.20495 ↗
36. 10.1002/jcc.2111210.1002/jcc.21112 ↗