Magnetic properties of theFe5SiB2−Fe5PB2system
Source abstract
Abstract
The magnetic properties of the compound ${\mathrm{Fe}}5{\mathrm{Si}}_{1\ensuremath{-}x}{\mathrm{P}}x{\mathrm{B}}2$ have been studied, with a focus on the Curie temperature ${T}_{\mathrm{C}}$, saturation magnetization ${M}_{\mathrm{S}}$, and magnetocrystalline anisotropy. Field and temperature dependent magnetization measurements were used to determine ${T}_{\mathrm{C}}\left(x\right)$ and ${M}_{\mathrm{S}}\left(x\right)$. The saturation magnetization at 10 K (300 K) is found to monotonically decrease from $1.11\phantom{\rule{0.28em}{0ex}}\mathrm{MA}/\mathrm{m}$ $(1.03\phantom{\rule{0.28em}{0ex}}\mathrm{MA}/\mathrm{m})$ to $0.97\phantom{\rule{0.28em}{0ex}}\mathrm{MA}/\mathrm{m}$ $(0.87\phantom{\rule{0.28em}{0ex}}\mathrm{MA}/\mathrm{m})$, as $x$ increases from 0 to 1. The Curie temperature is determined to be 810 and 615 K in ${\mathrm{Fe}}5{\mathrm{SiB}}2$ and ${\mathrm{Fe}}5{\mathrm{PB}}2$, respectively. The highest ${T}_{\mathrm{C}}$ is observed for $x=0.1$, while it decreases monotonically for larger $x$. The Curie temperatures have also been theoretically determined to be 700 and 660 K for ${\mathrm{Fe}}5{\mathrm{SiB}}2$ and ${\mathrm{Fe}}5{\mathrm{PB}}2$, respectively, using a combination of density functional theory and Monte Carlo simulations. The magnitude of the effective magnetocrystalline anisotropy was extracted using the law of approach to saturation, revealing an increase with increasing phosphorus concentration. Low-field magnetization vs temperature results for $x=0,0.1,0.2$ indicate that there is a transition from easy-axis to easy-plane anisotropy with decreasing temperature.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Rare-earth and actinide compounds · Iron-based superconductors research · Magnetic Properties of Alloys
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (24)
Show source-provided references
1. 10.1016/j.jssc.2015.12.01610.1016/j.jssc.2015.12.016 ↗
2. 10.1063/1.493449610.1063/1.4934496 ↗
3. 10.1103/PhysRevB.93.17441210.1103/PhysRevB.93.174412 ↗
4. 10.1016/j.jmmm.2015.10.08810.1016/j.jmmm.2015.10.088 ↗
5. 10.3891/acta.chem.scand.13-043310.3891/acta.chem.scand.13-0433 ↗
6. 10.1051/jphyscol:1976612210.1051/jphyscol:19766122 ↗
7. 10.1088/0034-4885/74/9/09650110.1088/0034-4885/74/9/096501 ↗
8. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
9. 10.1016/0022-4596(73)90021-210.1016/0022-4596(73)90021-2 ↗
10. 10.1107/S002188986900655810.1107/S0021889869006558 ↗
11. 10.1016/0921-4526(93)90108-I10.1016/0921-4526(93)90108-I ↗
12. 10.1180/minmag.1997.061.404.0710.1180/minmag.1997.061.404.07 ↗
13. S. Chikazumi · 199710.1093/oso/9780198517764.001.0001 ↗
14. 10.1103/PhysRevB.92.17441310.1103/PhysRevB.92.174413 ↗
15. 10.1088/0305-4608/14/7/00710.1088/0305-4608/14/7/007 ↗
16. 10.1016/0304-8853(86)90336-710.1016/0304-8853(86)90336-7 ↗
17. 10.1143/JPSJ.18.79710.1143/JPSJ.18.797 ↗
18. 10.1063/1.355678510.1063/1.3556785 ↗
19. 10.1103/PhysRevB.57.347810.1103/PhysRevB.57.3478 ↗
20. 10.1088/0953-8984/20/31/31520310.1088/0953-8984/20/31/315203 ↗
21. 10.1016/S0081-1947(08)60260-X10.1016/S0081-1947(08)60260-X ↗
22. J. M. D. Coey · 201010.1017/CBO9780511845000 ↗
23. 10.1016/S0925-8388(97)00127-810.1016/S0925-8388(97)00127-8 ↗
24. 10.1103/PhysRevB.86.08512510.1103/PhysRevB.86.085125 ↗