journal article·2020-10-19Open access

Strong magnetocaloric effect induced by spin reorientation transitions in epitaxial Ho thin films

O. Koplak, R. Morgunov, R. Medapalli, E. E. Fullerton, S. Mangin

Physical Review B· Volume 102· Issue 13

Abstract

Magnetocaloric effect (MCE) in an antiferromagnetic holmium (Ho) film is studied near the spin reorientation temperatures. A series of magnetization isotherms from 60 to 150 K around the N\'eel temperature, ${T}N\ensuremath{\approx}130\phantom{\rule{0.28em}{0ex}}\mathrm{K}$ were recorded for both in-plane and out-of-plane magnetic field orientations. A change in entropy, $\mathrm{\ensuremath{\Delta}}{S}M$ of $\text{--}5\phantom{\rule{0.28em}{0ex}}\mathrm{J}/\mathrm{kg}\mathrm{K}$ was found near ${T}N$ for an in-plane field orientation. A large change in $\mathrm{\ensuremath{\Delta}}{S}M$ of \ensuremath{-}11.8 J/kg K due to a fan-helix spin transition at $T=90\phantom{\rule{0.28em}{0ex}}\mathrm{K}$ is observed for an in-plane field orientation. Spin transition at both ${T}N$ and at the fan-helix transition exhibit larger MCE in the in-plane field orientations in comparison with the perpendicular orientation. The value of the refrigerant capacity extracted from the temperature dependence of $\mathrm{\ensuremath{\Delta}}{S}M(T)$ is found to be larger for the ``in- plane'' orientation by a factor of two.
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Research context

OpenAlex topics: Magnetic and transport properties of perovskites and related materials · Shape Memory Alloy Transformations · Advanced Condensed Matter Physics

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

References (39)

Show source-provided references
1. T. Chatterji · 2006
2. 10.1103/PhysRev.158.45010.1103/PhysRev.158.450 ↗
3. 10.1103/PhysRevB.40.1141410.1103/PhysRevB.40.11414 ↗
4. 10.1088/0305-4608/7/9/00510.1088/0305-4608/7/9/005 ↗
5. 10.1016/0378-4371(86)90241-410.1016/0378-4371(86)90241-4 ↗
6. 10.1016/j.jmmm.2014.10.02710.1016/j.jmmm.2014.10.027 ↗
7. 10.1088/0953-8984/10/30/01810.1088/0953-8984/10/30/018 ↗
8. 10.1088/0953-8984/27/14/14600210.1088/0953-8984/27/14/146002 ↗
9. 10.1016/j.actamat.2019.05.00410.1016/j.actamat.2019.05.004 ↗
10. 10.1038/nmat333410.1038/nmat3334 ↗
11. 10.1134/S106378341309026610.1134/S1063783413090266 ↗
12. 10.1016/j.physb.2017.03.03110.1016/j.physb.2017.03.031 ↗
13. 10.1103/PhysRev.127.204610.1103/PhysRev.127.2046 ↗
14. 10.1016/0921-4526(89)90026-410.1016/0921-4526(89)90026-4 ↗
15. E. E. Fullerton · 199710.1007/978-94-011-5478-9_48 ↗
16. 10.1016/S0368-2048(00)00318-210.1016/S0368-2048(00)00318-2 ↗
17. 10.1016/S0921-4526(99)01923-710.1016/S0921-4526(99)01923-7 ↗
18. 10.1107/S160057671600189810.1107/S1600576716001898 ↗
19. 10.1134/S102745101405042510.1134/S1027451014050425 ↗
20. 10.1088/0022-3727/5/1/30810.1088/0022-3727/5/1/308 ↗
21. 10.1063/1.472989310.1063/1.4729893 ↗
22. 10.1109/TMAG.2002.101776610.1109/TMAG.2002.1017766 ↗
23. C. D Jr. Graham · 1997
24. 10.1103/PhysRevB.34.345610.1103/PhysRevB.34.3456 ↗
25. 10.1016/0031-9163(64)91158-810.1016/0031-9163(64)91158-8 ↗
26. 10.1088/0953-8984/21/29/29600310.1088/0953-8984/21/29/296003 ↗
27. 10.1038/srep2239710.1038/srep22397 ↗
28. 10.1038/s41598-017-06728-510.1038/s41598-017-06728-5 ↗
29. 10.1088/0953-8984/21/23/23320110.1088/0953-8984/21/23/233201 ↗
30. 10.1103/PhysRevB.44.1237610.1103/PhysRevB.44.12376 ↗
31. 10.1143/JPSJ.71.173210.1143/JPSJ.71.1732 ↗
32. 10.1063/1.165632410.1063/1.1656324 ↗
33. 10.1103/PhysRevB.97.17441810.1103/PhysRevB.97.174418 ↗
34. 10.1016/j.ssc.2010.07.04910.1016/j.ssc.2010.07.049 ↗
35. 10.1038/s41598-019-49654-410.1038/s41598-019-49654-4 ↗
36. 10.1007/BF0081874910.1007/BF00818749 ↗
37. 10.1109/TMAG.2016.253013810.1109/TMAG.2016.2530138 ↗
38. 10.1103/PhysRevB.98.17442410.1103/PhysRevB.98.174424 ↗
39. 10.1088/0034-4885/68/6/R0410.1088/0034-4885/68/6/R04 ↗