journal article·2022-09-21Open access

Probing magnetic anisotropy and spin-reorientation transition in the three-dimensional antiferromagnet Ho0.5Dy0.5FeO3|Pt using spin Hall magnetoresistance

Aditya A. Wagh, Priyanka Garg, Arijit Haldar, Kingshuk Mallick, Tirthankar Chakraborty, Suja Elizabeth, P. S. Anil Kumar

Physical Review B· Volume 106· Issue 10

Abstract

Orthoferrites ($R{\mathrm{FeO}}3$) containing rare-earth ($R$) elements are 3D antiferromagnets (AFMs) that exhibit characteristic weak ferromagnetism originating due to slight canting of the spin moments and display a rich variety of spin-reorientation transitions in the magnetic field ($H$)-temperature ($T$) parameter space. We present spin Hall magnetoresistance (SMR) studies on a $b$ plate ($\mathit{ac}$ plane) of crystalline ${\mathrm{Ho}}0.5{\mathrm{Dy}}0.5{\mathrm{FeO}}3|\mathrm{Pt}$ hybrid at various $T$ in the range 11--300 K. In the room temperature ${\mathrm{\ensuremath{\Gamma}}}4$ phase, the switching between two degenerate domains occurs at fields above a critical value, ${H}_{\text{c}}\ensuremath{\approx}713$ Oe. Under $H>{H}_{\text{c}}$, the angular dependence of SMR ($\ensuremath{\alpha}$ scan) yielded a highly skewed curve with a sharp change (sign-reversal) along with a rotational hysteresis around the $\mathit{a}$ axis. Notably, at $H<{H}_{\text{c}}$, the $\ensuremath{\alpha}$-scan measurements on the single degenerate domain exhibited an anomalous sinusoidal signal of periodicity ${360}^{\ensuremath{\circ}}$. Low-$T$ evolution of the SMR curves ($H$ = 2.4 kOe) suggests weakening of the anisotropy possibly due to the $T$ evolution of Fe-$R$ exchange coupling. Below 25 K, the SMR modulation showed an abrupt change around the $\mathit{c}$ axis, marking the presence of a ${\mathrm{\ensuremath{\Gamma}}}2$ phase. We have employed a simple Hamiltonian and computed SMR to examine the observed skewed SMR modulation. In summary, SMR is found to be an effective tool to probe magnetic anisotropy as well as a spin reorientation in ${\mathrm{Ho}}0.5{\mathrm{Dy}}0.5{\mathrm{FeO}}3$. Our spin-transport study highlights the potential of ${\mathrm{Ho}}0.5{\mathrm{Dy}}0.5{\mathrm{FeO}}3$ for future AFM spintronic devices.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Multiferroics and related materials · Magnetic properties of thin films · Physics of Superconductivity and Magnetism

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

References (52)

Show source-provided references
1. 10.1038/s41427-019-0135-910.1038/s41427-019-0135-9 ↗
2. 10.1103/RevModPhys.90.01500510.1103/RevModPhys.90.015005 ↗
3. 10.1016/j.physleta.2018.01.00810.1016/j.physleta.2018.01.008 ↗
4. 10.1038/s41567-018-0063-610.1038/s41567-018-0063-6 ↗
5. 10.1002/adma.20190560310.1002/adma.201905603 ↗
6. 10.1038/nnano.2016.1810.1038/nnano.2016.18 ↗
7. 10.1126/science.aab103110.1126/science.aab1031 ↗
8. 10.1103/PhysRevLett.124.02720210.1103/PhysRevLett.124.027202 ↗
9. 10.1038/s41928-020-0425-910.1038/s41928-020-0425-9 ↗
10. 10.1103/PhysRevB.98.02040810.1103/PhysRevB.98.020408 ↗
11. 10.1063/1.501841110.1063/1.5018411 ↗
12. 10.1063/1.511654910.1063/1.5116549 ↗
13. 10.1103/PhysRevB.98.13442610.1103/PhysRevB.98.134426 ↗
14. 10.1103/PhysRevLett.118.14720210.1103/PhysRevLett.118.147202 ↗
15. 10.1063/1.498637210.1063/1.4986372 ↗
16. 10.1103/PhysRevB.94.13441810.1103/PhysRevB.94.134418 ↗
17. 10.1038/s42005-019-0150-810.1038/s42005-019-0150-8 ↗
18. 10.1103/PhysRevB.97.01441710.1103/PhysRevB.97.014417 ↗
19. 10.1063/5.000952910.1063/5.0009529 ↗
20. 10.1103/PhysRevLett.110.20660110.1103/PhysRevLett.110.206601 ↗
21. 10.1103/PhysRevB.87.14441110.1103/PhysRevB.87.144411 ↗
22. 10.1088/0953-8984/28/10/10300410.1088/0953-8984/28/10/103004 ↗
23. 10.1103/PhysRevB.102.09443710.1103/PhysRevB.102.094437 ↗
24. 10.1021/acs.nanolett.9b0245910.1021/acs.nanolett.9b02459 ↗
25. 10.1103/PhysRevB.104.02441510.1103/PhysRevB.104.024415 ↗
26. 10.1103/PhysRevB.100.22440310.1103/PhysRevB.100.224403 ↗
27. 10.1103/PhysRevB.103.14440610.1103/PhysRevB.103.144406 ↗
28. 10.1103/PhysRevLett.118.06720210.1103/PhysRevLett.118.067202 ↗
29. 10.1063/1.495957310.1063/1.4959573 ↗
30. 10.1103/PhysRevB.102.10442010.1103/PhysRevB.102.104420 ↗
31. 10.1016/j.jallcom.2013.08.12910.1016/j.jallcom.2013.08.129 ↗
32. 10.1103/PhysRevLett.112.03720310.1103/PhysRevLett.112.037203 ↗
33. 10.1103/PhysRevLett.101.09720510.1103/PhysRevLett.101.097205 ↗
34. 10.1016/j.jallcom.2018.07.06110.1016/j.jallcom.2018.07.061 ↗
35. 10.1088/1361-648X/ab303c10.1088/1361-648X/ab303c ↗
36. 10.1070/PU1976v019n07ABEH00527410.1070/PU1976v019n07ABEH005274 ↗
37. 10.1103/PhysRevB.103.02442310.1103/PhysRevB.103.024423 ↗
38. 10.1107/S056773946800030610.1107/S0567739468000306 ↗
39. 10.1103/PhysRevB.103.13440610.1103/PhysRevB.103.134406 ↗
40. 10.1021/acs.jpcc.9b0898510.1021/acs.jpcc.9b08985 ↗
41. 10.1016/j.jallcom.2019.15204310.1016/j.jallcom.2019.152043 ↗
42. 10.1016/j.jcrysgro.2010.11.01410.1016/j.jcrysgro.2010.11.014 ↗
43. 10.1016/j.jmmm.2020.16685510.1016/j.jmmm.2020.166855 ↗
44. 10.1016/j.jmmm.2018.05.00210.1016/j.jmmm.2018.05.002 ↗
45. 10.1143/JPSJ.34.33810.1143/JPSJ.34.338 ↗
46. 10.1016/S0022-3697(74)80003-X10.1016/S0022-3697(74)80003-X ↗
47. 10.1088/1361-648X/aac06b10.1088/1361-648X/aac06b ↗
48. 10.1063/1.165963110.1063/1.1659631 ↗
49. 10.1103/PhysRevB.69.10442910.1103/PhysRevB.69.104429 ↗
50. 10.1103/PhysRevB.98.06442410.1103/PhysRevB.98.064424 ↗
51. 10.1103/PhysRevB.80.13441610.1103/PhysRevB.80.134416 ↗
52. 10.1063/1.491634210.1063/1.4916342 ↗