journal article·2013-01-01Open access

Promising ferrimagnetic double perovskite oxides towards high spin polarization at high temperature

Si-Da Li, Peng Chen, Bang-Gui Liu

AIP Advances· Volume 3· Issue 1

Abstract

We predict through our first-principles calculations that four double perovskite oxides of Bi2ABO6 (AB = FeMo, MnMo, MnOs, CrOs) are half-metallic ferrimagnets. Our calculated results shows that the four optimized structures have negative formation energy, from -0.42 to -0.26 eV per formula unit, which implies that they could probably be realized. In the case of Bi2FeMoO6, the half-metallic gap and Curie temperature are predicted to reach to 0.71 eV and 650 K, respectively, which indicates that high spin polarization could be kept at high temperatures far beyond room temperature. It is believed that some of them could be synthesized soon and would prove useful for spintronic applications.
Source: crossref · Quality: baseline

Research context

OpenAlex topics: Multiferroics and related materials · Heusler alloys: electronic and magnetic properties · Magnetic and transport properties of perovskites and related materials

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

Affiliations

Chinese Academy of Sciences 1 Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, , Beijing 100190, China

University of Science and Technology of China 2 Department of Physics & School of Gifted Youth, , Hefei 230026, China

Funding

National Natural Science Foundation of China

References (25)

Show source-provided references
1. Science · 2001 · 294 · 148810.1126/science.1065389 ↗
2. Nat. Mater. · 2009 · 8 · 5610.1038/nmat2341 ↗
3. Phys. Rev. Lett. · 1983 · 50 · 202410.1103/PhysRevLett.50.2024 ↗
4. Nature (London) · 1998 · 392 · 79410.1038/33883 ↗
5. Nature (London) · 1998 · 395 · 67710.1038/26427 ↗
6. Appl. Phys. Lett. · 2006 · 89 · 10290210.1063/1.2346258 ↗
7. Appl. Phys. Lett. · 2011 · 99 · 18350510.1063/1.3657528 ↗
8. Phys. Rev. Lett. · 2012 · 109 · 15720710.1103/PhysRevLett.109.157207 ↗
9. Phys. Rev. B · 2012 · 85 · 16120110.1103/PhysRevB.85.161201 ↗
10. J. Phys. Conden. Matter · 2007 · 19 · 02320110.1088/0953-8984/19/2/023201 ↗
11. J. Phys. D · 2012 · 45 · 03300110.1088/0022-3727/45/3/033001 ↗
12. Phys. Rev. · 1964 · 136 · B86410.1103/PhysRev.136.B864 ↗
13. Phys. Rev. · 1965 · 140 · A113310.1103/PhysRev.140.A1133 ↗
14. Phys. Rev. B · 1993 · 47 · 55810.1103/PhysRevB.47.558 ↗
15. Phys. Rev. B · 1996 · 54 · 1116910.1103/PhysRevB.54.11169 ↗
16. Phys. Rev. Lett. · 1996 · 77 · 386510.1103/PhysRevLett.77.3865 ↗
17. J. Phys. C · 1980 · 13 · 267510.1088/0022-3719/13/14/009 ↗
18. Phys. Rev. B · 1976 · 13 · 518810.1103/PhysRevB.13.5188 ↗
19. J. Chem. Phys. · 1953 · 21 · 108710.1063/1.1699114 ↗
20. 2002
21. Appl. Phys. Lett. · 2005 · 86 · 01250510.1063/1.1843290 ↗
22. Phys. Rev. B · 2005 · 72 · 21410510.1103/PhysRevB.72.214105 ↗
23. Phys. Rev. B · 2003 · 67 · 17241110.1103/PhysRevB.67.172411 ↗
24. Phys. Rev. Lett. · 2003 · 91 · 03720410.1103/PhysRevLett.91.037204 ↗
25. Galanakis · 2005 · 26710.1007/b137760 ↗