Equation of motion and the constraining field in ab initio spin dynamics
Source abstract
Abstract
In $a\phantom{\rule{0}{0ex}}b$ $i\phantom{\rule{0}{0ex}}n\phantom{\rule{0}{0ex}}i\phantom{\rule{0}{0ex}}t\phantom{\rule{0}{0ex}}i\phantom{\rule{0}{0ex}}o$ spin dynamics, the effective field acting on a magnetic moment can either be calculated from the energy gradient or from the negative of the constraining field that stabilizes an out-of-equilibrium noncollinear magnetic configuration. Here, the authors show that the constraining field in DFT calculations is not exactly the negative of the effective magnetic field obtained from the energy gradient. They provide a theoretical explanation of this surprising result and discuss the implications for $a\phantom{\rule{0}{0ex}}b$ $i\phantom{\rule{0}{0ex}}n\phantom{\rule{0}{0ex}}i\phantom{\rule{0}{0ex}}t\phantom{\rule{0}{0ex}}i\phantom{\rule{0}{0ex}}o$ spin dynamics.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Physics of Superconductivity and Magnetism · Advanced Chemical Physics Studies · Spectroscopy and Quantum Chemical Studies
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (32)
Show source-provided references
1. G. Bertotti · 2009
2. O. Eriksson · 201710.1093/oso/9780198788669.001.0001 ↗
3. 10.1103/PhysRevLett.111.12720410.1103/PhysRevLett.111.127204 ↗
4. 10.1103/PhysRevB.96.14441310.1103/PhysRevB.96.144413 ↗
5. 10.1103/PhysRevLett.76.425010.1103/PhysRevLett.76.4250 ↗
6. 10.1103/PhysRevLett.52.99710.1103/PhysRevLett.52.997 ↗
7. 10.1103/PhysRevLett.75.72910.1103/PhysRevLett.75.729 ↗
8. 10.1103/PhysRevB.54.101910.1103/PhysRevB.54.1019 ↗
9. 10.1080/1364281980820677510.1080/13642819808206775 ↗
10. 10.1063/1.37049410.1063/1.370494 ↗
11. 10.1103/PhysRevLett.53.251210.1103/PhysRevLett.53.2512 ↗
12. 10.1103/PhysRevB.71.21443510.1103/PhysRevB.71.214435 ↗
13. 10.1103/PhysRevB.58.29310.1103/PhysRevB.58.293 ↗
14. L. D. Landau · Phys. Z. Sowjet. · 1935 · 8 · 153
15. 10.1103/PhysRevB.95.13444710.1103/PhysRevB.95.134447 ↗
16. 10.1103/PhysRevB.91.05442010.1103/PhysRevB.91.054420 ↗
17. 10.17586/2220-8054-2020-11-1-65-7710.17586/2220-8054-2020-11-1-65-77 ↗
18. 10.1103/PhysRevA.72.02450210.1103/PhysRevA.72.024502 ↗
19. 10.1103/PhysRevB.69.02441510.1103/PhysRevB.69.024415 ↗
20. 10.1088/2515-7639/aae7db10.1088/2515-7639/aae7db ↗
21. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
22. 10.1016/0927-0256(96)00008-010.1016/0927-0256(96)00008-0 ↗
23. 10.1103/PhysRevB.63.10040110.1103/PhysRevB.63.100401 ↗
24. 10.1088/0305-4608/14/7/00710.1088/0305-4608/14/7/007 ↗
25. 10.1016/0304-8853(87)90721-910.1016/0304-8853(87)90721-9 ↗
26. 10.1103/PhysRevLett.90.08720510.1103/PhysRevLett.90.087205 ↗
27. H. Hellmann · 1937
28. 10.1103/PhysRev.56.34010.1103/PhysRev.56.340 ↗
29. 10.1103/PhysRev.140.A113310.1103/PhysRev.140.A1133 ↗
30. 10.1103/PhysRev.94.149810.1103/PhysRev.94.1498 ↗
31. 10.1088/1367-2630/16/1/01303210.1088/1367-2630/16/1/013032 ↗
32. 10.1088/0953-8984/18/29/01810.1088/0953-8984/18/29/018 ↗