Fluctuation-induced interactions and the spin-glass transition in Fe2TiO5
Source abstract
Abstract
We investigate the spin-glass transition in the strongly frustrated well-known compound ${\mathrm{Fe}}2{\mathrm{TiO}}5$. A remarkable feature of this transition, widely discussed in the literature, is its anisotropic properties: The transition manifests itself in the magnetic susceptibly only along one axis, despite ${\mathrm{Fe}}3+ {d}5$ spins having no orbital component. We demonstrate, using neutron scattering, that below the transition temperature ${T}g=55$ K, ${\mathrm{Fe}}2{\mathrm{TiO}}5$ develops nanoscale surfboard-shaped antiferromagnetic regions in which the ${\mathrm{Fe}}3+$ spins are aligned perpendicular to the axis which exhibits freezing. We show that the glass transition may result from the freezing of transverse fluctuations of the magnetization of these regions and we develop a mean-field replica theory of such a transition, revealing a type of magnetic van der Waals effect.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Theoretical and Computational Physics · Advanced Condensed Matter Physics · Multiferroics and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Physics Department, University of California Santa Cruz, Santa Cruz, California 95064, USA
Materials Science Division, Argonne National Laboratory, Lemont, Illinois 60439, USA
NHMFL, Florida State University, Tallahassee, Florida 32310, USA
Neutron Scattering Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37830, USA
Department of Chemical and Biomedical Engineering, FAMU-FSU College of Engineering, Tallahassee, Florida 32310, USA
Funding
U.S. Department of Energy · National Science Foundation · Basic Energy Sciences
References (25)
Show source-provided references
1. A. Abragam · 1970
2. 10.1051/jphyscol:197110610.1051/jphyscol:1971106 ↗
3. 10.1080/0001873970010155810.1080/00018739700101558 ↗
4. 10.1103/RevModPhys.58.80110.1103/RevModPhys.58.801 ↗
5. 10.1016/0022-5088(78)90040-110.1016/0022-5088(78)90040-1 ↗
6. 10.1103/PhysRevLett.43.78210.1103/PhysRevLett.43.782 ↗
7. 10.1103/PhysRevLett.53.62010.1103/PhysRevLett.53.620 ↗
8. 10.1103/PhysRevB.31.319110.1103/PhysRevB.31.3191 ↗
9. 10.1103/PhysRevB.68.14440410.1103/PhysRevB.68.144404 ↗
10. 10.1016/j.jallcom.2019.05.34310.1016/j.jallcom.2019.05.343 ↗
11. 10.1088/0022-3719/18/17/00110.1088/0022-3719/18/17/001 ↗
12. 10.1063/1.34114510.1063/1.341145 ↗
13. 10.1007/s12043-008-0259-x10.1007/s12043-008-0259-x ↗
14. 10.1107/S160057671800403X10.1107/S160057671800403X ↗
15. 10.1016/j.nima.2014.07.02910.1016/j.nima.2014.07.029 ↗
16. 10.1107/S160057671600136910.1107/S1600576716001369 ↗
17. S. W. Lovesey · 1984
18. H. E. Stanley · 1971
19. 10.1088/0031-8949/20/1/01910.1088/0031-8949/20/1/019 ↗
20. 10.3367/UFNr.0163.199306a.000110.3367/UFNr.0163.199306a.0001 ↗
21. M. Mezard · 198610.1142/0271 ↗
22. 10.1088/1742-5468/2008/02/L0200110.1088/1742-5468/2008/02/L02001 ↗
23. 10.1103/PhysRevB.73.22443210.1103/PhysRevB.73.224432 ↗
24. 10.1038/nature0444710.1038/nature04447 ↗
25. 10.1016/S0370-1573(01)00015-110.1016/S0370-1573(01)00015-1 ↗