journal article·2016-07-25Open access

Emergence of competing magnetic interactions induced by Ge doping in the semiconductorFeGa3

J. C. Alvarez-Quiceno, M. Cabrera-Baez, R. A. Ribeiro, M. A. Avila, G. M. Dalpian, J. M. Osorio-Guillén

Physical Review B· Volume 94· Issue 1

Abstract

${\mathrm{FeGa}}3$ is an unusual intermetallic semiconductor that presents intriguing magnetic responses to the tuning of its electronic properties. When doped with Ge, the system evolves from diamagnetic to paramagnetic to ferromagnetic ground states that are not well understood. In this work, we have performed a joint theoretical and experimental study of ${\mathrm{FeGa}}_{3\ensuremath{-}x}{\mathrm{Ge}}x$ using density functional theory and magnetic susceptibility measurements. For low Ge concentrations we observe the formation of localized moments on some Fe atoms and, as the dopant concentration increases, a more delocalized magnetic behavior emerges. The magnetic configuration strongly depends on the dopant distribution, leading even to the appearance of antiferromagnetic interactions in certain configurations.
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Research context

OpenAlex topics: Magnetic and transport properties of perovskites and related materials · Magnetic properties of thin films · Iron-based superconductors research

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References (26)

Show source-provided references
1. 10.1063/1.180394710.1063/1.1803947 ↗
2. 10.1063/1.358584310.1063/1.3585843 ↗
3. 10.1007/s11664-013-2888-110.1007/s11664-013-2888-1 ↗
4. 10.1103/PhysRevB.86.23520210.1103/PhysRevB.86.235202 ↗
5. 10.1007/s11664-013-2932-110.1007/s11664-013-2932-1 ↗
6. 10.1103/PhysRevB.82.15520210.1103/PhysRevB.82.155202 ↗
7. 10.1103/PhysRevB.89.19510210.1103/PhysRevB.89.195102 ↗
8. 10.1143/JPSJ.77.02470510.1143/JPSJ.77.024705 ↗
9. 10.1143/JPSJ.78.01370210.1143/JPSJ.78.013702 ↗
10. 10.1103/PhysRevB.88.06442210.1103/PhysRevB.88.064422 ↗
11. 10.1088/1742-6596/200/1/01201410.1088/1742-6596/200/1/012014 ↗
12. 10.1007/s11003-013-9601-710.1007/s11003-013-9601-7 ↗
13. 10.1103/PhysRevB.89.10442610.1103/PhysRevB.89.104426 ↗
14. 10.1103/PhysRevB.86.14442110.1103/PhysRevB.86.144421 ↗
15. 10.1080/1364281920821507310.1080/13642819208215073 ↗
16. 10.1080/14786435.2012.68217910.1080/14786435.2012.682179 ↗
17. 10.1103/PhysRevLett.100.13640610.1103/PhysRevLett.100.136406 ↗
18. 10.1103/PhysRevB.57.150510.1103/PhysRevB.57.1505 ↗
19. 10.1103/PhysRevB.62.1639210.1103/PhysRevB.62.16392 ↗
20. 10.1103/PhysRevB.50.1795310.1103/PhysRevB.50.17953 ↗
21. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
22. 10.1103/PhysRevB.59.175810.1103/PhysRevB.59.1758 ↗
23. 10.1006/jssc.2001.950310.1006/jssc.2001.9503 ↗
24. 10.1103/PhysRevB.85.20120210.1103/PhysRevB.85.201202 ↗
25. 10.1016/j.physb.2005.01.31710.1016/j.physb.2005.01.317 ↗
26. 10.1103/PhysRevB.93.06441010.1103/PhysRevB.93.064410 ↗