Crossover from an incommensurate singlet spiral state with a vanishingly small spin gap to a valence-bond solid state in dimerized frustrated ferromagnetic spin chains
Source abstract
Abstract
Motivated by the magnetic properties of the spin-chain compounds ${\mathrm{LiCuSbO}}4\ensuremath{\equiv}{\mathrm{LiSbCuO}}4$ and ${\mathrm{Rb}}2{\mathrm{Cu}}2{\mathrm{Mo}}3{\mathrm{O}}12$, we study the ground state of the Heisenberg chain with dimerized nearest-neighbor ferromagnetic (FM) (${J}1,{J}1^{\ensuremath{'}}<0$) and next-nearest-neighbor antiferromagnetic (${J}2>0$) couplings. Using the density-matrix renormalization group technique and spin-wave theory, we find a first-order transition between a fully polarized FM and an incommensurate spiral state at $2\ensuremath{\alpha}=\ensuremath{\beta}/(1+\ensuremath{\beta})$, where $\ensuremath{\alpha}$ is the frustration ratio ${J}2/|{J}1|$ and $\ensuremath{\beta}$ the degree of dimerization ${J}1^{\ensuremath{'}}/{J}1$. In the singlet spiral state the spin-gap is vanishingly small in the vicinity of the FM transition, corresponding to a situation of ${\mathrm{LiCuSbO}}4$. For larger $\ensuremath{\alpha}$, corresponding to ${\mathrm{Rb}}2{\mathrm{Cu}}2{\mathrm{Mo}}3{\mathrm{O}}12$, and smaller $\ensuremath{\beta}$ there is a crossover from this frustration induced incommensurate state to an Affleck-Lieb-Kennedy-Tasaki-type valence-bond solid state with substantial spin gaps.
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Research context
OpenAlex topics: Advanced Condensed Matter Physics · Physics of Superconductivity and Magnetism · Magnetic and transport properties of perovskites and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (36)
Show source-provided references
1. 10.1063/1.218627810.1063/1.2186278 ↗
2. 10.1038/nature0891710.1038/nature08917 ↗
3. 10.1103/PhysRevLett.98.10720410.1103/PhysRevLett.98.107204 ↗
4. 10.1103/PhysRevLett.77.364910.1103/PhysRevLett.77.3649 ↗
5. 10.1103/PhysRevB.91.06040710.1103/PhysRevB.91.060407 ↗
6. 10.1103/PhysRevB.44.469310.1103/PhysRevB.44.4693 ↗
7. 10.1209/0295-5075/92/3700110.1209/0295-5075/92/37001 ↗
8. 10.1103/PhysRevLett.109.02720310.1103/PhysRevLett.109.027203 ↗
9. 10.7566/JPSJ.82.09470910.7566/JPSJ.82.094709 ↗
10. 10.1103/PhysRevB.90.13440110.1103/PhysRevB.90.134401 ↗
11. 10.1103/PhysRevB.92.21441510.1103/PhysRevB.92.214415 ↗
12. 10.1103/PhysRevB.70.10442610.1103/PhysRevB.70.104426 ↗
13. Y. Yasui · JPS Conf. Proc. · 2014 · 3 · 014014
14. 10.1103/PhysRevLett.70.365110.1103/PhysRevLett.70.3651 ↗
15. 10.1103/PhysRevB.89.02440710.1103/PhysRevB.89.024407 ↗
16. 10.1103/PhysRevB.19.355610.1103/PhysRevB.19.3556 ↗
17. 10.1103/PhysRevB.78.17441210.1103/PhysRevB.78.174412 ↗
18. 10.1088/0953-8984/7/45/01610.1088/0953-8984/7/45/016 ↗
19. 10.1103/PhysRevLett.81.91010.1103/PhysRevLett.81.910 ↗
20. 10.1103/PhysRevB.63.22442310.1103/PhysRevB.63.224423 ↗
21. 10.1016/0375-9601(83)90631-X10.1016/0375-9601(83)90631-X ↗
22. 10.1103/PhysRevLett.50.115310.1103/PhysRevLett.50.1153 ↗
23. 10.1143/JPSJ.60.134710.1143/JPSJ.60.1347 ↗
24. 10.1143/JPSJ.62.284510.1143/JPSJ.62.2845 ↗
25. 10.1103/PhysRevLett.59.79910.1103/PhysRevLett.59.799 ↗
26. 10.1103/PhysRevLett.69.286310.1103/PhysRevLett.69.2863 ↗
27. 10.1088/0953-8984/3/19/01310.1088/0953-8984/3/19/013 ↗
28. 10.1103/PhysRevB.91.04512110.1103/PhysRevB.91.045121 ↗
29. 10.1103/PhysRevB.86.09441710.1103/PhysRevB.86.094417 ↗
30. 10.1103/PhysRevB.54.986210.1103/PhysRevB.54.9862 ↗
31. 10.1143/JPSJS.74S.4210.1143/JPSJS.74S.42 ↗
32. 10.1103/PhysRevB.53.R295910.1103/PhysRevB.53.R2959 ↗
33. 10.1103/PhysRevB.54.1005410.1103/PhysRevB.54.10054 ↗
34. 10.1103/PhysRevB.45.402710.1103/PhysRevB.45.4027 ↗
35. 10.1103/PhysRevB.65.15511310.1103/PhysRevB.65.155113 ↗
36. 10.1209/epl/i2005-10020-810.1209/epl/i2005-10020-8 ↗