The strain induced band gap modulation from narrow gap semiconductor to half-metal on Ti2CrGe: A first principles study
Source abstract
Abstract
The Heusler alloy Ti2CrGe is a stable L21 phase with antiferromagnetic ordering. With band-gap energy (∼ 0.18 eV) obtained from a first-principles calculation, it belongs to the group of narrow band gap semiconductor. The band-gap energy decreases with increasing lattice compression and disappears until a strain of −5%; moreover, gap contraction only occurs in the spin-down states, leading to half-metallic character at the −5% strain. The Ti1, Ti2, and Cr moments all exhibit linear changes in behavior within strains of −5%– +5%. Nevertheless, the total zero moment is robust for these strains. The imaginary part of the dielectric function for both up and down spin states shows a clear onset energy, indicating a corresponding electronic gap for the two spin channels.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Heusler alloys: electronic and magnetic properties · MXene and MAX Phase Materials · 2D Materials and Applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Hebei University of Technology 1 School of Science, , Tianjin 300401, People’s Republic of China
Hebei University of Technology 2 Research Institute for Energy Equipment Materials, , Tianjin 300401, People’s Republic of China
Funding
the Youth Research Foundation of Science and Technology for Colleges and Universities of Hebei Province · National Natural Science Foundation of China · Natural Science Foundation of Hebei Province
References (31)
Show source-provided references
1. Phys. Rev. Lett. · 2008 · 100 · 15640410.1103/PhysRevLett.100.156404 ↗
2. Phys. Rev. Lett. · 1983 · 50 · 202410.1103/PhysRevLett.50.2024 ↗
3. von Klitzing · 1996
4. Appl. Phys. Lett. · 2013 · 102 · 02240210.1063/1.4775599 ↗
5. Phys. Rev. B · 2004 · 69 · 14441310.1103/PhysRevB.69.144413 ↗
6. Science · 1998 · 281 · 95110.1126/science.281.5379.951 ↗
7. Phys. Rev. Lett. · 1995 · 74 · 117110.1103/PhysRevLett.74.1171 ↗
8. Phys. Rev. Lett. · 2006 · 97 · 02640110.1103/PhysRevLett.97.026401 ↗
9. Appl. Phys. Lett. · 2013 · 103 · 14240410.1063/1.4823820 ↗
10. J. Phys.: Condens. Matter · 2014 · 26 · 08600310.1088/0953-8984/26/8/086003 ↗
11. Appl. Phys. Lett. · 2011 · 99 · 05250910.1063/1.3619844 ↗
12. J. Magn. Magn. Mater. · 2009 · 321 · L3410.1016/j.jmmm.2009.01.006 ↗
13. J. Phys. D: Appl. Phys. · 2007 · 40 · 150710.1088/0022-3727/40/6/S01 ↗
14. J. Magn. Magn. Matter. · 2008 · 320 · 134510.1016/j.jmmm.2007.11.006 ↗
15. J. of Appl. Phys. · 2009 · 105 · 08371710.1063/1.3116533 ↗
16. Appl. Phys. Lett. · 2009 · 94 · 24250210.1063/1.3156811 ↗
17. Phys. Rev. B · 1996 · 54 · 1116910.1103/PhysRevB.54.11169 ↗
18. Comput. Mater. Sci. · 1996 · 6 · 1510.1016/0927-0256(96)00008-0 ↗
19. Phys. Rev. Lett. · 1996 · 77 · 386510.1103/PhysRevLett.77.3865 ↗
20. Phys. Rev. B · 1992 · 46 · 667110.1103/PhysRevB.46.6671 ↗
21. Phys. Rev. B · 1994 · 50 · 1795310.1103/PhysRevB.50.17953 ↗
22. Phys. Rev. B · 1997 · 55 · 1035510.1103/PhysRevB.55.10355 ↗
23. Phys. Rev. B · 2008 · 78 · 13410610.1103/PhysRevB.78.134106 ↗
24. Phys. Rev. B · 2011 · 84 · 09430210.1103/PhysRevB.84.094302 ↗
25. Phys. Rev. B · 2012 · 86 · 21430110.1103/PhysRevB.86.214301 ↗
26. Phys. Rev. B · 2015 · 91 · 09430610.1103/PhysRevB.91.094306 ↗
27. Phys. Rev. B · 2006 · 73 · 04511210.1103/PhysRevB.73.045112 ↗
28. Acta Phys. Sin. · 2015 · 64 · 07710410.7498/aps.64.077104 ↗
29. 1985
30. Phys. Rev. B · 2007 · 76 · 05411510.1103/PhysRevB.76.054115 ↗
31. Phys. Rev. B · 2005 · 72 · 03520410.1103/PhysRevB.72.035204 ↗