journal article·2021-12-29Open access

Approximate two-body generating Hamiltonian for the particle-hole Pfaffian wave function

Kiryl Pakrouski

Physical Review B· Volume 104· Issue 24

Abstract

We present two two-body Hamiltonians that approximate the exact particle-hole Pfaffian wave function with their ground states for all the system sizes where this wave function has been numerically constructed to date. The approximate wave functions have high overlap with the original and reproduce well the low-lying entanglement spectrum and structure factor. The approximate generating Hamiltonians are obtained by an optimization procedure where three to four pseudopotentials are varied in the neighbourhood of second Landau level Coulomb interaction or of a noninteracting model. They belong to a finite region in the variational space of Hamiltonians where each point approximately generates the particle-hole Pfaffian. We diagonalize the identified Hamiltonians for up to 20 electrons and find that for them the particle-hole Pfaffian shift appears energetically more favorable. The possibility to interpret the data in terms of composite fermions is discussed.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Quantum and electron transport phenomena · Physics of Superconductivity and Magnetism · Quantum, superfluid, helium dynamics

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

Affiliations

Institute for Theoretical Physics, ETH Zurich, 8093 Zurich, Switzerland and Department of Physics, Princeton University, Princeton, New Jersey 08544, USA

Funding

U.S. Department of Energy · Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung · Swiss National Supercomputing Centre

References (65)

Show source-provided references
1. 10.1103/PhysRevLett.59.177610.1103/PhysRevLett.59.1776 ↗
2. 10.1142/S021797929000013910.1142/S0217979290000139 ↗
3. 10.1142/S021797929200084010.1142/S0217979292000840 ↗
4. 10.1103/RevModPhys.80.108310.1103/RevModPhys.80.1083 ↗
5. 10.1103/RevModPhys.89.02500510.1103/RevModPhys.89.025005 ↗
6. 10.1016/0550-3213(91)90407-O10.1016/0550-3213(91)90407-O ↗
7. 10.1103/PhysRevLett.99.23680610.1103/PhysRevLett.99.236806 ↗
8. 10.1103/PhysRevLett.99.23680710.1103/PhysRevLett.99.236807 ↗
9. 10.1103/PhysRevX.5.02100410.1103/PhysRevX.5.021004 ↗
10. 10.1103/PhysRevB.87.24512910.1103/PhysRevB.87.245129 ↗
11. 10.1103/PhysRevLett.105.09680210.1103/PhysRevLett.105.096802 ↗
12. 10.1103/PhysRevLett.119.02680110.1103/PhysRevLett.119.026801 ↗
13. 10.1103/PhysRevB.87.15542610.1103/PhysRevB.87.155426 ↗
14. 10.1103/PhysRevLett.106.11680110.1103/PhysRevLett.106.116801 ↗
15. 10.1103/PhysRevB.91.04511510.1103/PhysRevB.91.045115 ↗
16. 10.1103/PhysRevX.5.03102710.1103/PhysRevX.5.031027 ↗
17. 10.1103/PhysRevLett.99.03680510.1103/PhysRevLett.99.036805 ↗
18. 10.1038/s41586-018-0184-110.1038/s41586-018-0184-1 ↗
19. 10.1103/PhysRevB.98.08110710.1103/PhysRevB.98.081107 ↗
20. 10.1103/PhysRevB.98.03512710.1103/PhysRevB.98.035127 ↗
21. 10.1103/PhysRevB.102.19515310.1103/PhysRevB.102.195153 ↗
22. 10.1103/PhysRevLett.80.150510.1103/PhysRevLett.80.1505 ↗
23. 10.1103/PhysRevLett.84.468510.1103/PhysRevLett.84.4685 ↗
24. 10.1103/PhysRevLett.100.16680310.1103/PhysRevLett.100.166803 ↗
25. 10.1103/PhysRevLett.101.01680710.1103/PhysRevLett.101.016807 ↗
26. 10.1103/PhysRevB.77.16531610.1103/PhysRevB.77.165316 ↗
27. 10.1103/PhysRevB.83.19513510.1103/PhysRevB.83.195135 ↗
28. 10.1103/PhysRevLett.117.09680210.1103/PhysRevLett.117.096802 ↗
29. 10.1103/PhysRevB.97.12140610.1103/PhysRevB.97.121406 ↗
30. 10.1103/PhysRevB.98.04511210.1103/PhysRevB.98.045112 ↗
31. 10.1103/PhysRevLett.121.02680110.1103/PhysRevLett.121.026801 ↗
32. 10.1103/PhysRevB.97.16512410.1103/PhysRevB.97.165124 ↗
33. 10.1103/PhysRevB.101.04130210.1103/PhysRevB.101.041302 ↗
34. 10.1103/PhysRevB.98.16740110.1103/PhysRevB.98.167401 ↗
35. 10.1103/PhysRevB.98.16740210.1103/PhysRevB.98.167402 ↗
36. 10.1103/PhysRevB.99.08530910.1103/PhysRevB.99.085309 ↗
37. 10.1103/PhysRevLett.125.15770210.1103/PhysRevLett.125.157702 ↗
38. 10.1103/PhysRevLett.125.23680210.1103/PhysRevLett.125.236802 ↗
39. 10.1103/PhysRevLett.124.12680110.1103/PhysRevLett.124.126801 ↗
40. 10.1103/PhysRevB.102.20510410.1103/PhysRevB.102.205104 ↗
41. 10.1103/PhysRevLett.125.01680110.1103/PhysRevLett.125.016801 ↗
42. 10.1103/PhysRevB.104.L08140710.1103/PhysRevB.104.L081407 ↗
43. 10.1103/PhysRevB.34.267010.1103/PhysRevB.34.2670 ↗
44. 10.1103/PhysRevLett.51.60510.1103/PhysRevLett.51.605 ↗
45. 10.1103/PhysRevB.41.937710.1103/PhysRevB.41.9377 ↗
46. 10.22331/q-2020-09-02-31510.22331/q-2020-09-02-315 ↗
47. 10.1103/PhysRevLett.122.04050410.1103/PhysRevLett.122.040504 ↗
48. 10.1103/PhysRevX.8.03102910.1103/PhysRevX.8.031029 ↗
49. 10.1103/PhysRevB.98.08111310.1103/PhysRevB.98.081113 ↗
50. 10.22331/q-2019-07-08-15910.22331/q-2019-07-08-159 ↗
51. 10.1103/PhysRevLett.96.24680510.1103/PhysRevLett.96.246805 ↗
52. 10.1103/PhysRevLett.101.01050410.1103/PhysRevLett.101.010504 ↗
53. 10.1103/PhysRevLett.54.58110.1103/PhysRevLett.54.581 ↗
54. 10.1103/PhysRevB.33.248110.1103/PhysRevB.33.2481 ↗
55. F. D. M. Haldane · 1990
56. 10.1103/PhysRevLett.104.07680310.1103/PhysRevLett.104.076803 ↗
57. 10.1103/PhysRevLett.63.19910.1103/PhysRevLett.63.199 ↗
58. 10.1103/PhysRevB.87.24542510.1103/PhysRevB.87.245425 ↗
59. 10.1103/PhysRevB.98.11510710.1103/PhysRevB.98.115107 ↗
60. 10.1103/PhysRevB.100.19530310.1103/PhysRevB.100.195303 ↗
61. 10.1142/S021798492030004510.1142/S0217984920300045 ↗
62. 10.1103/PhysRevLett.125.23060210.1103/PhysRevLett.125.230602 ↗
63. 10.1103/PhysRevResearch.3.04315610.1103/PhysRevResearch.3.043156 ↗
64. 10.1038/s41567-021-01230-210.1038/s41567-021-01230-2 ↗
65. 10.1103/PhysRevB.102.12130310.1103/PhysRevB.102.121303 ↗