journal article·2019-08-05Open access

Suppression of the bulk high spin–low spin transition by doping the chiral magnet MnGe

N. Martin, M. Deutsch, T. C. Hansen, M. T. Fernandez-Diaz, L. N. Fomicheva, A. V. Tsvyashchenko, I. Mirebeau

Physical Review B· Volume 100· Issue 6

Abstract

In the MnGe chiral magnet, the helimagnetic order and local moment collapse in two steps, showing the succession of high spin (HS) and low spin (LS) states as pressure increases. Here, we use high-pressure neutron diffraction to study the doped compounds ${\mathrm{Mn}}0.86{\mathrm{Co}}0.14\mathrm{Ge}$ and ${\mathrm{Mn}}0.9{\mathrm{Rh}}0.1\mathrm{Ge}$, and show that the evolution of their microscopic magnetic properties is instead continuous. It means that the bulk HS-LS transition is a unique feature of pure MnGe, very sensitive to small changes of the band structure and easily suppressed by chemical substitution. On the other hand, the helimagnetic correlations appear to be strengthened by doping and survive up to larger pressures ($\ensuremath{\approx}19\phantom{\rule{0.28em}{0ex}}\mathrm{GPa}$, to be compared with $\ensuremath{\approx}13\phantom{\rule{0.28em}{0ex}}\mathrm{GPa}$). We discuss these results in the light of other disordered systems with remarkable properties, the so-called Invar alloys.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Magnetic and transport properties of perovskites and related materials · Magnetic properties of thin films · Advanced Condensed Matter Physics

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

References (35)

Show source-provided references
1. 10.1088/0370-1328/82/2/31410.1088/0370-1328/82/2/314 ↗
2. 10.1103/PhysRevB.41.693910.1103/PhysRevB.41.6939 ↗
3. C. E. Guillaume · C. R. Hebd. Séances Acad. Sci. · 1897 · 125 · 235
4. 10.1021/ic801257410.1021/ic8012574 ↗
5. 10.1021/ja000348u10.1021/ja000348u ↗
6. J. Kishine · 2015
7. 10.1038/nature0223210.1038/nature02232 ↗
8. 10.1103/PhysRevLett.114.01680310.1103/PhysRevLett.114.016803 ↗
9. 10.1103/PhysRevLett.106.15660310.1103/PhysRevLett.106.156603 ↗
10. 10.1103/PhysRevB.85.20520510.1103/PhysRevB.85.205205 ↗
11. 10.1103/PhysRevB.99.10040210.1103/PhysRevB.99.100402 ↗
12. 10.1103/PhysRevB.89.18040710.1103/PhysRevB.89.180407 ↗
13. 10.1103/PhysRevB.93.21440410.1103/PhysRevB.93.214404 ↗
14. 10.1088/1742-6596/391/1/01210410.1088/1742-6596/391/1/012104 ↗
15. E. Wasserman · 1990
16. 10.1103/PhysRevB.80.06442110.1103/PhysRevB.80.064421 ↗
17. 10.1103/PhysRevB.96.02041310.1103/PhysRevB.96.020413 ↗
18. A. Tsvyashchenko · 2012
19. 10.1088/0957-0233/19/3/03400110.1088/0957-0233/19/3/034001 ↗
20. S. Klotz · 201210.1201/b13074 ↗
21. 10.1016/0921-4526(93)90108-I10.1016/0921-4526(93)90108-I ↗
22. 10.1103/PhysRevB.90.14440110.1103/PhysRevB.90.144401 ↗
23. 10.1103/PhysRevB.93.17440510.1103/PhysRevB.93.174405 ↗
24. 10.1103/PhysRevB.98.12512110.1103/PhysRevB.98.125121 ↗
25. 10.1038/s41467-019-08985-610.1038/s41467-019-08985-6 ↗
26. 10.1038/2184810.1038/21848 ↗
27. 10.1103/PhysRevLett.86.485110.1103/PhysRevLett.86.4851 ↗
28. 10.1103/PhysRevB.88.21440210.1103/PhysRevB.88.214402 ↗
29. 10.1103/PhysRevB.71.05440210.1103/PhysRevB.71.054402 ↗
30. 10.1103/PhysRevB.76.01443410.1103/PhysRevB.76.014434 ↗
31. 10.1016/j.intermet.2013.12.00910.1016/j.intermet.2013.12.009 ↗
32. 10.1016/S0925-8388(03)00591-710.1016/S0925-8388(03)00591-7 ↗
33. 10.1209/0295-5075/111/1700810.1209/0295-5075/111/17008 ↗
34. 10.1063/1.185541910.1063/1.1855419 ↗
35. 10.1080/0895795090341819410.1080/08957950903418194 ↗