journal article·2021-11-19Open access

Density-matrix renormalization group study of optical conductivity of the Mott insulator for two-dimensional clusters

Kazuya Shinjo, Yoshiki Tamaki, Shigetoshi Sota, Takami Tohyama

Physical Review B· Volume 104· Issue 20

Abstract

The real part of optical conductivity $\text{Re}\ensuremath{\sigma}(\ensuremath{\omega})$ of the Mott insulators has a large amount of information on how spin and charge degrees of freedom interact with each other. By using the time-dependent density-matrix renormalization group, we study $\text{Re}\ensuremath{\sigma}(\ensuremath{\omega})$ of the two-dimensional Hubbard model on a square lattice at half filling. We find an excitonic peak at the Mott-gap edge of $\text{Re}\ensuremath{\sigma}(\ensuremath{\omega})$ not only for the two-dimensional square lattice but also for two- and four-leg ladders. For the square lattice, however, we do not clearly find a gap between an excitonic peak and continuum band, which indicates that a bound state is not well defined. The emergence of an excitonic peak in $\text{Re}\ensuremath{\sigma}(\ensuremath{\omega})$ implies the formation of a spin polaron. Examining the dependence of $\text{Re}\ensuremath{\sigma}(\ensuremath{\omega})$ on the on-site Coulomb interaction and next-nearest-neighbor hoppings, we confirm that an excitonic peak is generated from a magnetic effect. Electron scattering due to an electron-phonon interaction is expected to easily suppress an excitonic peak since spectral width of an excitonic peak is very narrow. Introducing a large broadening in $\text{Re}\ensuremath{\sigma}(\ensuremath{\omega})$ by modeling the electron-phonon coupling present in ${\mathrm{La}}2{\mathrm{CuO}}4$ and ${\mathrm{Nd}}2{\mathrm{CuO}}4$, we obtain $\text{Re}\ensuremath{\sigma}(\ensuremath{\omega})$ comparable with experiments.
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Research context

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

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Affiliations

Department of Applied Physics, Tokyo University of Science, Tokyo 125-8585, Japan

Computational Materials Science Research Team, RIKEN Center for Computational Science (R-CCS), Kobe, Hyogo 650-0047, Japan

Funding

Core Research for Evolutional Science and Technology · Japan Society for the Promotion of Science · Ministry of Education, Culture, Sports, Science and Technology · Japan Science and Technology Corporation · Precursory Research for Embryonic Science and Technology · RIKEN · Hokkaido University · University of Tokyo

References (38)

Show source-provided references
1. 10.1103/PhysRevB.41.232610.1103/PhysRevB.41.2326 ↗
2. F. H. L. Essler · 200510.1017/CBO9780511534843 ↗
3. 10.1103/PhysRevB.69.24511710.1103/PhysRevB.69.245117 ↗
4. 10.1103/PhysRevB.100.23513410.1103/PhysRevB.100.235134 ↗
5. 10.1103/PhysRevB.43.794210.1103/PhysRevB.43.7942 ↗
6. 10.1103/PhysRevB.52.976010.1103/PhysRevB.52.9760 ↗
7. 10.1126/sciadv.aav218710.1126/sciadv.aav2187 ↗
8. 10.1103/PhysRevB.45.1010710.1103/PhysRevB.45.10107 ↗
9. 10.1103/PhysRevB.72.04511310.1103/PhysRevB.72.045113 ↗
10. 10.1143/JPSJ.76.03470510.1143/JPSJ.76.034705 ↗
11. 10.1103/PhysRevB.85.08512410.1103/PhysRevB.85.085124 ↗
12. 10.1088/1367-2630/18/10/10300410.1088/1367-2630/18/10/103004 ↗
13. 10.1126/science.aau706310.1126/science.aau7063 ↗
14. 10.1103/PhysRevB.54.R1726910.1103/PhysRevB.54.R17269 ↗
15. 10.1080/1364281970820570210.1080/13642819708205702 ↗
16. 10.1103/PhysRevB.64.12511910.1103/PhysRevB.64.125119 ↗
17. 10.1103/PhysRevB.67.07510610.1103/PhysRevB.67.075106 ↗
18. 10.1103/PhysRevB.103.03514110.1103/PhysRevB.103.035141 ↗
19. 10.1016/j.aop.2019.16799810.1016/j.aop.2019.167998 ↗
20. 10.1103/PhysRevB.100.04511010.1103/PhysRevB.100.045110 ↗
21. 10.1103/PhysRevB.58.179410.1103/PhysRevB.58.1794 ↗
22. 10.1103/PhysRevB.64.15511210.1103/PhysRevB.64.155112 ↗
23. 10.1103/PhysRevLett.75.92610.1103/PhysRevLett.75.926 ↗
24. 10.1103/PhysRevB.53.1172110.1103/PhysRevB.53.11721 ↗
25. 10.1103/PhysRevX.5.04104110.1103/PhysRevX.5.041041 ↗
26. 10.1103/PhysRevLett.77.510210.1103/PhysRevLett.77.5102 ↗
27. 10.1103/PhysRevB.46.1385210.1103/PhysRevB.46.13852 ↗
28. 10.1103/PhysRevB.45.223710.1103/PhysRevB.45.2237 ↗
29. 10.1103/PhysRevB.73.20512110.1103/PhysRevB.73.205121 ↗
30. 10.1103/PhysRevB.63.16511010.1103/PhysRevB.63.165110 ↗
31. 10.1103/PhysRevB.64.23510210.1103/PhysRevB.64.235102 ↗
32. 10.1103/PhysRevB.77.13443710.1103/PhysRevB.77.134437 ↗
33. 10.1103/PhysRevB.98.13450110.1103/PhysRevB.98.134501 ↗
34. 10.1016/0921-4526(91)90624-N10.1016/0921-4526(91)90624-N ↗
35. 10.1103/PhysRevB.52.723010.1103/PhysRevB.52.7230 ↗
36. G. D. Mahan · 2013
37. 10.1103/PhysRevLett.93.07640110.1103/PhysRevLett.93.076401 ↗
38. 10.1143/JPSJ.76.05400410.1143/JPSJ.76.054004 ↗