journal article·2023-12-06Open access

Linear colossal magnetoresistance and magnetic textures in LaTiO3 thin films on SrTiO3

Teresa Tschirner, Berengar Leikert, Felix Kern, Daniel Wolf, Axel Lubk, Martin Kamp, Kirill Miller, Fabian Hartmann, Sven Höfling, Judith Gabel, Matthias Schmitt, Martin Stübinger, Julia Küspert, Tien-Lin Lee, Bernd Büchner, Joseph Dufouleur, Marc Gabay, Michael Sing, Ralph Claessen, Louis Veyrat

Physical Review B· Volume 108· Issue 24

Abstract

Linear magnetoresistance (LMR) is of particular interest for memory, electronics, and sensing applications, especially when it does not saturate over a wide range of magnetic fields. Structural disorder, however, also tends to limit the mobility and hence the overall LMR amplitude. An alternative route to achieve large LMR is via nonstructural inhomogeneities which do not affect the zero field mobility, like magnetic domains. Here, we report a colossal positive linear magnetoresistance in $\mathrm{La}{\mathrm{TiO}}3/\mathrm{Sr}{\mathrm{TiO}}3$ heterostructures, with amplitude up to 6500% at 9T at low temperature. The colossal amplitude of the LMR, one of the largest in oxide heterostructure, stems from the unusual combination of a very high heterostructure mobility, up to 40 000 ${\mathrm{cm}}2\phantom{\rule{0.16em}{0ex}}{\mathrm{V}}^{\ensuremath{-}1}\phantom{\rule{0.16em}{0ex}}{\mathrm{s}}^{\ensuremath{-}1}$, and a very large coverage of low-mobility regions. Low-temperature Lorentz transmission electron microscopy measurements further reveals a striped magnetic structure at the sub-$\textmu{}\mathrm{m}$ scale in the $\mathrm{La}{\mathrm{TiO}}3$ layer, compatible with in-plane spiral magnetism, with very high surface coverage. We propose that the low-mobility regions and striped magnetic regions are correlated, we model the increase in scattering induced by the magnetic texture, and we show that the non saturating LMR fits the Parish-Littlewood scenario. Our results provide a novel route for the engineering of large-LMR systems, using magnetic texture.
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Research context

OpenAlex topics: Magnetic and transport properties of perovskites and related materials · Electronic and Structural Properties of Oxides · Advanced Condensed Matter Physics

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

References (69)

Show source-provided references
1. 10.1103/PhysRevB.58.278810.1103/PhysRevB.58.2788 ↗
2. D. D. Majumder · 2013
3. 10.1126/science.264.5157.41310.1126/science.264.5157.413 ↗
4. 10.1103/PhysRevB.94.22440410.1103/PhysRevB.94.224404 ↗
5. 10.1103/PhysRevB.68.12510710.1103/PhysRevB.68.125107 ↗
6. 10.1063/1.35811910.1063/1.358119 ↗
7. 10.1126/science.273.5271.8110.1126/science.273.5271.81 ↗
8. 10.1103/PhysRevLett.76.135610.1103/PhysRevLett.76.1356 ↗
9. 10.1103/PhysRevX.10.04106210.1103/PhysRevX.10.041062 ↗
10. 10.1021/acs.chemmater.1c0359610.1021/acs.chemmater.1c03596 ↗
11. 10.1002/pssb.20190013910.1002/pssb.201900139 ↗
12. 10.1103/PhysRevB.86.03544210.1103/PhysRevB.86.035442 ↗
13. 10.1103/PhysRevLett.106.15680810.1103/PhysRevLett.106.156808 ↗
14. D. Shoenberg · 198410.1017/CBO9780511897870 ↗
15. S. Datta · 1997
16. 10.1038/nature0207310.1038/nature02073 ↗
17. 10.1103/PhysRevB.72.09441710.1103/PhysRevB.72.094417 ↗
18. 10.1038/ncomms210610.1038/ncomms2106 ↗
19. 10.1021/acs.nanolett.1c0319810.1021/acs.nanolett.1c03198 ↗
20. 10.1103/PhysRevB.92.18020410.1103/PhysRevB.92.180204 ↗
21. 10.1088/1361-648X/ab8d7410.1088/1361-648X/ab8d74 ↗
22. 10.1063/1.495427210.1063/1.4954272 ↗
23. 10.1038/3630610.1038/36306 ↗
24. 10.1038/417421a10.1038/417421a ↗
25. 10.1103/PhysRevLett.88.06660210.1103/PhysRevLett.88.066602 ↗
26. 10.1103/PhysRevB.91.04120310.1103/PhysRevB.91.041203 ↗
27. 10.1103/PhysRevX.5.03102310.1103/PhysRevX.5.031023 ↗
28. 10.1209/0295-5075/114/2700210.1209/0295-5075/114/27002 ↗
29. 10.1103/PhysRevLett.114.11720110.1103/PhysRevLett.114.117201 ↗
30. 10.1103/PhysRevB.92.08130610.1103/PhysRevB.92.081306 ↗
31. 10.1103/PhysRevB.104.L16140410.1103/PhysRevB.104.L161404 ↗
32. 10.1209/epl/i2000-00220-210.1209/epl/i2000-00220-2 ↗
33. 10.1021/nl101797d10.1021/nl101797d ↗
34. 10.1063/1.370127710.1063/1.3701277 ↗
35. 10.1021/acsami.6b1304410.1021/acsami.6b13044 ↗
36. 10.1038/s41467-021-24692-710.1038/s41467-021-24692-7 ↗
37. 10.1002/admi.20210123510.1002/admi.202101235 ↗
38. 10.1038/s41535-021-00354-110.1038/s41535-021-00354-1 ↗
39. 10.1063/1.235442210.1063/1.2354422 ↗
40. 10.1038/ncomms108410.1038/ncomms1084 ↗
41. 10.1088/0953-8984/9/39/00510.1088/0953-8984/9/39/005 ↗
42. 10.1038/s41467-018-04014-010.1038/s41467-018-04014-0 ↗
43. 10.1021/acs.nanolett.6b0206010.1021/acs.nanolett.6b02060 ↗
44. 10.1063/5.003257210.1063/5.0032572 ↗
45. 10.1038/srep3429510.1038/srep34295 ↗
46. 10.1038/s41598-018-26017-z10.1038/s41598-018-26017-z ↗
47. 10.1103/PhysRevB.80.11520710.1103/PhysRevB.80.115207 ↗
48. 10.1103/PhysRevB.75.21420310.1103/PhysRevB.75.214203 ↗
49. 10.1063/1.490117510.1063/1.4901175 ↗
50. 10.1016/j.ultramic.2019.01.00510.1016/j.ultramic.2019.01.005 ↗
51. 10.1038/s41567-018-0363-x10.1038/s41567-018-0363-x ↗
52. 10.1038/nmat375310.1038/nmat3753 ↗
53. 10.1103/PhysRevB.59.1183210.1103/PhysRevB.59.11832 ↗
54. 10.1103/PhysRevB.71.14441210.1103/PhysRevB.71.144412 ↗
55. 10.1051/jphys:01985004601050010.1051/jphys:019850046010500 ↗
56. 10.1038/nphys270210.1038/nphys2702 ↗
57. 10.1038/nphys273710.1038/nphys2737 ↗
58. 10.1103/PhysRevB.77.11535010.1103/PhysRevB.77.115350 ↗
59. 10.1038/srep1025510.1038/srep10255 ↗
60. 10.1126/sciadv.abf963110.1126/sciadv.abf9631 ↗
61. 10.1002/adma.20170670810.1002/adma.201706708 ↗
62. 10.1002/sia.152610.1002/sia.1526 ↗
63. 10.1103/PhysRev.80.40110.1103/PhysRev.80.401 ↗
64. 10.1103/PhysRev.118.119010.1103/PhysRev.118.1190 ↗
65. 10.1038/s41467-021-25037-010.1038/s41467-021-25037-0 ↗
66. A. Lubk · 2018
67. 10.1103/PhysRevB.96.08513210.1103/PhysRevB.96.085132 ↗
68. 10.1038/nmat156910.1038/nmat1569 ↗
69. 10.1103/PhysRevB.73.21442610.1103/PhysRevB.73.214426 ↗