Neural-network-supported basis optimizer for the configuration interaction problem in quantum many-body clusters: Feasibility study and numerical proof
Source abstract
Abstract
A neural-network approach to optimize the selection of Slater determinants in configuration interaction calculations for condensed-matter quantum many-body systems is developed. We exemplify our algorithm on the discrete version of the single-impurity Anderson model with up to 299 bath sites. Employing a neural network classifier and active learning, our algorithm enhances computational efficiency by iteratively identifying the most relevant Slater determinants for the ground state wave function. We benchmark our results against established methods and investigate the efficiency of our approach compared to another basis truncation scheme without a neural network. Our algorithm demonstrates a substantial improvement in the efficiency of determinant selection, yielding a more compact and computationally manageable basis without compromising accuracy. Given the straightforward application of our neural-network-supported selection scheme to other model Hamiltonians of quantum many-body clusters, our algorithm can significantly advance selective configuration interaction calculations in the context of correlated condensed matter.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Quantum, superfluid, helium dynamics · Advanced Chemical Physics Studies · Quantum many-body systems
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Max Planck Institute for the Science of Light
Friedrich-Alexander-Universität Erlangen-Nürnberg
Heidelberg University
University of Würzburg
Funding
Friedrich-Alexander-Universität Erlangen-Nürnberg · Deutsche Forschungsgemeinschaft
References (51)
Show source-provided references
1. A. Szabo · 2012
2. 10.1016/S0009-2614(99)00791-510.1016/S0009-2614(99)00791-5 ↗
3. 10.1103/PhysRevLett.62.32410.1103/PhysRevLett.62.324 ↗
4. 10.1103/PhysRevB.45.647910.1103/PhysRevB.45.6479 ↗
5. 10.1103/RevModPhys.68.1310.1103/RevModPhys.68.13 ↗
6. 10.1103/PhysRevB.62.R928310.1103/PhysRevB.62.R9283 ↗
7. 10.1103/PhysRevLett.87.18640110.1103/PhysRevLett.87.186401 ↗
8. 10.1007/s00214010028510.1007/s002140100285 ↗
9. 10.1063/1.167919910.1063/1.1679199 ↗
10. 10.1006/jcph.1998.595310.1006/jcph.1998.5953 ↗
11. 10.1063/1.504450310.1063/1.5044503 ↗
12. 10.1021/acs.jctc.8b0053610.1021/acs.jctc.8b00536 ↗
13. 10.1021/acs.jctc.8b0084910.1021/acs.jctc.8b00849 ↗
14. 10.1021/acs.jctc.1c0076910.1021/acs.jctc.1c00769 ↗
15. 10.1021/acs.jctc.1c0019610.1021/acs.jctc.1c00196 ↗
16. 10.1021/acs.jctc.1c0001010.1021/acs.jctc.1c00010 ↗
17. 10.1021/acs.jctc.2c0121610.1021/acs.jctc.2c01216 ↗
18. 10.1021/acs.jctc.9b0082810.1021/acs.jctc.9b00828 ↗
19. 10.1103/PhysRevC.105.03430610.1103/PhysRevC.105.034306 ↗
20. 10.1103/PhysRevLett.131.13300210.1103/PhysRevLett.131.133002 ↗
21. 10.1103/PhysRevA.110.04281810.1103/PhysRevA.110.042818 ↗
22. 10.1103/PhysRev.124.4110.1103/PhysRev.124.41 ↗
23. 10.1103/PhysRevB.85.23510710.1103/PhysRevB.85.235107 ↗
24. 10.1103/PhysRevB.90.08510210.1103/PhysRevB.90.085102 ↗
25. 10.1103/PhysRevB.104.11511910.1103/PhysRevB.104.115119 ↗
26. 10.1103/RevModPhys.91.04500210.1103/RevModPhys.91.045002 ↗
27. 10.1021/acs.jpca.3c0532210.1021/acs.jpca.3c05322 ↗
28. 10.1126/science.aag230210.1126/science.aag2302 ↗
29. 10.1126/sciadv.abl685010.1126/sciadv.abl6850 ↗
30. 10.7566/JPSJ.86.09300110.7566/JPSJ.86.093001 ↗
31. 10.1038/s41467-020-15724-910.1038/s41467-020-15724-9 ↗
32. 10.1103/PhysRevLett.108.25300210.1103/PhysRevLett.108.253002 ↗
33. 10.1063/1.500723010.1063/1.5007230 ↗
34. 10.1038/s41467-020-17265-710.1038/s41467-020-17265-7 ↗
35. 10.1038/s41467-017-00839-310.1038/s41467-017-00839-3 ↗
36. 10.1103/PhysRevLett.125.07640210.1103/PhysRevLett.125.076402 ↗
37. 10.1038/s41524-023-01115-310.1038/s41524-023-01115-3 ↗
38. 10.1103/PhysRevB.109.04515310.1103/PhysRevB.109.045153 ↗
39. 10.1016/j.aichem.2023.10004210.1016/j.aichem.2023.100042 ↗
40. 10.1063/5.013339910.1063/5.0133399 ↗
41. 10.1103/PhysRevB.90.15513610.1103/PhysRevB.90.155136 ↗
42. 10.1103/PhysRevB.101.24110510.1103/PhysRevB.101.241105 ↗
43. 10.1103/PhysRevB.104.20512010.1103/PhysRevB.104.205120 ↗
44. 10.1103/PhysRevB.103.24511810.1103/PhysRevB.103.245118 ↗
45. 10.3390/cryst1209126910.3390/cryst12091269 ↗
46. K. P. Murphy · 2022
47. I. Goodfellow · 2016
48. M. Abadi · 2016
49. 10.1103/PhysRevB.85.16511310.1103/PhysRevB.85.165113 ↗
50. A. Geron · 2019
51. 10.1088/0953-8984/20/34/34520510.1088/0953-8984/20/34/345205 ↗