journal article·2016-09-06Open access

Disordered dimer state in electron-dopedSr3Ir2O7

Tom Hogan, Rebecca Dally, Mary Upton, J. P. Clancy, Kenneth Finkelstein, Young-June Kim, M. J. Graf, Stephen D. Wilson

Physical Review B· Volume 94· Issue 10

Abstract

Spin excitations are explored in the electron-doped spin-orbit Mott insulator ${({\mathrm{Sr}}_{1\ensuremath{-}x}{\mathrm{La}}x)}3{\mathrm{Ir}}2{\mathrm{O}}7$. As this bilayer square lattice system is doped into the metallic regime, long-range antiferromagnetism vanishes, yet a spectrum of gapped spin excitation remains. Excitation lifetimes are strongly damped with increasing carrier concentration, and the energy-integrated spectral weight becomes nearly momentum independent as static spin order is suppressed. Local magnetic moments, absent in the parent system, grow in metallic samples and approach values consistent with one $J=\frac{1}{2}$ impurity per electron doped. Our combined data suggest that the magnetic spectra of metallic ${({\mathrm{Sr}}_{1\ensuremath{-}x}{\mathrm{La}}x)}3{\mathrm{Ir}}2{\mathrm{O}}7$ are best described by excitations out of a disordered dimer state.
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Research context

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

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References (35)

Show source-provided references
1. 10.1103/PhysRevLett.72.277710.1103/PhysRevLett.72.2777 ↗
2. 10.1143/JPSJ.65.59410.1143/JPSJ.65.594 ↗
3. 10.1103/PhysRevLett.78.301910.1103/PhysRevLett.78.3019 ↗
4. 10.1103/PhysRevLett.80.579010.1103/PhysRevLett.80.5790 ↗
5. 10.1103/PhysRevB.51.1648310.1103/PhysRevB.51.16483 ↗
6. 10.1103/PhysRevB.61.347510.1103/PhysRevB.61.3475 ↗
7. 10.1103/PhysRevB.69.22441610.1103/PhysRevB.69.224416 ↗
8. 10.1103/PhysRevB.85.18041110.1103/PhysRevB.85.180411 ↗
9. 10.1103/PhysRevLett.95.20720610.1103/PhysRevLett.95.207206 ↗
10. 10.1103/PhysRevLett.87.21720110.1103/PhysRevLett.87.217201 ↗
11. 10.1103/PhysRevB.54.1617210.1103/PhysRevB.54.16172 ↗
12. 10.1103/PhysRevB.55.835710.1103/PhysRevB.55.8357 ↗
13. 10.1016/0025-5408(94)90120-110.1016/0025-5408(94)90120-1 ↗
14. 10.1103/PhysRevLett.102.01720510.1103/PhysRevLett.102.017205 ↗
15. 10.1103/PhysRevLett.112.02640310.1103/PhysRevLett.112.026403 ↗
16. 10.1103/PhysRevLett.108.17700310.1103/PhysRevLett.108.177003 ↗
17. 10.1088/0953-8984/24/31/31220210.1088/0953-8984/24/31/312202 ↗
18. 10.1103/PhysRevLett.109.03720410.1103/PhysRevLett.109.037204 ↗
19. 10.1103/PhysRevB.86.10040110.1103/PhysRevB.86.100401 ↗
20. 10.1103/PhysRevLett.109.15740210.1103/PhysRevLett.109.157402 ↗
21. 10.1103/PhysRevB.92.02440510.1103/PhysRevB.92.024405 ↗
22. 10.1103/PhysRevB.59.11110.1103/PhysRevB.59.111 ↗
23. 10.1103/PhysRevB.52.352110.1103/PhysRevB.52.3521 ↗
24. 10.1103/PhysRevLett.114.25720310.1103/PhysRevLett.114.257203 ↗
25. 10.1103/PhysRevB.92.07512510.1103/PhysRevB.92.075125 ↗
26. 10.1088/0953-8984/19/13/13621410.1088/0953-8984/19/13/136214 ↗
27. 10.1103/PhysRevB.84.02040310.1103/PhysRevB.84.020403 ↗
28. 10.1103/PhysRevB.93.24110210.1103/PhysRevB.93.241102 ↗
29. 10.1103/PhysRevB.52.770810.1103/PhysRevB.52.7708 ↗
30. 10.1143/JPSJ.65.238510.1143/JPSJ.65.2385 ↗
31. 10.1103/PhysRevLett.86.108610.1103/PhysRevLett.86.1086 ↗
32. 10.1103/PhysRevLett.103.04720110.1103/PhysRevLett.103.047201 ↗
33. 10.1103/PhysRevB.93.13411010.1103/PhysRevB.93.134110 ↗
34. 10.1103/PhysRevB.60.1520110.1103/PhysRevB.60.15201 ↗
35. 10.1103/PhysRevLett.106.13640210.1103/PhysRevLett.106.136402 ↗