journal article·2021-08-09

Resummation-based quantum Monte Carlo for quantum paramagnetic phases

Nisheeta Desai, Sumiran Pujari

Physical Review B· Volume 104· Issue 6
Publisher page

Abstract

For spin rotational symmetric models with a positive-definite high-temperature expansion of the partition function, a stochastic sampling of the series expansion upon partial resummation becomes logically equivalent to sampling an uncolored closely packed loop-gas model in one higher dimension. Based on this, we devise quantum Monte Carlo updates that importance-sample loop configurations for general $SU(N)$ in fundamental and higher-symmetric representations. The algorithmic performance systematically improves with an increase in (continuous) $N$, allowing the efficient simulation of quantum paramagnets. The underlying reason for the increased efficacy is the correspondence of quantum paramagnetic phases such as valence bond solids to short-loop phases on the loop-gas side rather than the particular value of $N$. This also gives a connection between Sandvik's $JQ$ model class and classical loop-gas models in the deconfined universality class.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Physics of Superconductivity and Magnetism · Theoretical and Computational Physics · Advanced Condensed Matter Physics

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

Affiliations

Department of Theoretical Physics, Tata Institute of Fundamental Research, Mumbai, MH 400005, India

Department of Physics, Indian Institute of Technology Bombay, Mumbai, MH 400076, India

Funding

National Science Foundation · Science and Engineering Research Board

References (53)

Show source-provided references
1. A. W. Sandvik · 2019
2. 10.1146/annurev-conmatphys-030212-18421510.1146/annurev-conmatphys-030212-184215 ↗
3. 10.1103/PhysRevLett.54.96610.1103/PhysRevLett.54.966 ↗
4. 10.1103/PhysRevLett.61.102910.1103/PhysRevLett.61.1029 ↗
5. 10.1103/PhysRevLett.62.169410.1103/PhysRevLett.62.1694 ↗
6. 10.1016/0550-3213(89)90061-810.1016/0550-3213(89)90061-8 ↗
7. 10.1103/PhysRevB.42.456810.1103/PhysRevB.42.4568 ↗
8. 10.1103/PhysRevLett.66.177310.1103/PhysRevLett.66.1773 ↗
9. 10.1103/PhysRevLett.61.237610.1103/PhysRevLett.61.2376 ↗
10. 10.1143/PTP.58.137710.1143/PTP.58.1377 ↗
11. 10.1103/PhysRevLett.77.513010.1103/PhysRevLett.77.5130 ↗
12. 10.1103/PhysRevB.43.595010.1103/PhysRevB.43.5950 ↗
13. 10.1088/0305-4470/25/13/01710.1088/0305-4470/25/13/017 ↗
14. A. W. Sandvik · 2010
15. 10.1103/PhysRevLett.95.20720310.1103/PhysRevLett.95.207203 ↗
16. 10.1103/PhysRevB.80.18440110.1103/PhysRevB.80.184401 ↗
17. 10.1103/PhysRevLett.70.87510.1103/PhysRevLett.70.875 ↗
18. 10.1016/0375-9601(93)90603-W10.1016/0375-9601(93)90603-W ↗
19. 10.1103/PhysRevLett.73.129510.1103/PhysRevLett.73.1295 ↗
20. 10.1103/PhysRevB.59.R1415710.1103/PhysRevB.59.R14157 ↗
21. 10.1080/000187302100004919510.1080/0001873021000049195 ↗
22. 10.1103/PhysRevB.82.02440710.1103/PhysRevB.82.024407 ↗
23. 10.1134/1.55866110.1134/1.558661 ↗
24. 10.1103/PhysRevE.66.04670110.1103/PhysRevE.66.046701 ↗
25. 10.1103/PhysRevE.68.05670110.1103/PhysRevE.68.056701 ↗
26. 10.1103/PhysRevE.71.03670610.1103/PhysRevE.71.036706 ↗
27. 10.1103/PhysRevLett.95.12720610.1103/PhysRevLett.95.127206 ↗
28. 10.1103/PhysRevLett.97.14720210.1103/PhysRevLett.97.147202 ↗
29. 10.1088/0953-8984/19/14/14520310.1088/0953-8984/19/14/145203 ↗
30. 10.1103/PhysRevB.93.23510310.1103/PhysRevB.93.235103 ↗
31. 10.1103/PhysRevLett.58.8610.1103/PhysRevLett.58.86 ↗
32. 10.1103/PhysRevLett.62.36110.1103/PhysRevLett.62.361 ↗
33. 10.1103/PhysRevB.91.05441310.1103/PhysRevB.91.054413 ↗
34. 10.1103/PhysRevLett.107.11060110.1103/PhysRevLett.107.110601 ↗
35. 10.1103/PhysRevB.88.13441110.1103/PhysRevB.88.134411 ↗
36. 10.1103/PhysRevX.5.04104810.1103/PhysRevX.5.041048 ↗
37. 10.1007/BF0210880510.1007/BF02108805 ↗
38. 10.1007/BF0217835810.1007/BF02178358 ↗
39. 10.1143/PTP.56.145410.1143/PTP.56.1454 ↗
40. 10.1103/PhysRevLett.123.10720210.1103/PhysRevLett.123.107202 ↗
41. 10.1103/PhysRevB.84.05440710.1103/PhysRevB.84.054407 ↗
42. 10.1103/PhysRevLett.90.11720310.1103/PhysRevLett.90.117203 ↗
43. 10.1007/BF0121802110.1007/BF01218021 ↗
44. 10.1103/PhysRevB.99.16513510.1103/PhysRevB.99.165135 ↗
45. 10.1103/PhysRevB.103.09442110.1103/PhysRevB.103.094421 ↗
46. 10.1103/PhysRevLett.87.04720310.1103/PhysRevLett.87.047203 ↗
47. 10.1143/JPSJ.73.137910.1143/JPSJ.73.1379 ↗
48. 10.1103/PhysRevLett.98.05720210.1103/PhysRevLett.98.057202 ↗
49. 10.1103/PhysRevB.92.13440410.1103/PhysRevB.92.134404 ↗
50. 10.1016/j.nuclphysb.2006.05.03210.1016/j.nuclphysb.2006.05.032 ↗
51. 10.1103/PhysRevLett.98.22720210.1103/PhysRevLett.98.227202 ↗
52. 10.1126/science.109180610.1126/science.1091806 ↗
53. 10.1103/PhysRevB.70.14440710.1103/PhysRevB.70.144407 ↗