journal article·2018-04-12Open access

Numerical renormalization group method for entanglement negativity at finite temperature

Jeongmin Shim, H.-S. Sim, Seung-Sup B. Lee

Physical Review B· Volume 97· Issue 15

Abstract

We develop a numerical method to compute the negativity, an entanglement measure for mixed states, between the impurity and the bath in quantum impurity systems at finite temperature. We construct a thermal density matrix by using the numerical renormalization group (NRG), and evaluate the negativity by implementing the NRG approximation that reduces computational cost exponentially. We apply the method to the single-impurity Kondo model and the single-impurity Anderson model. In the Kondo model, the negativity exhibits a power-law scaling at temperature much lower than the Kondo temperature and a sudden death at high temperature. In the Anderson model, the charge fluctuation of the impurity contributes to the negativity even at zero temperature when the on-site Coulomb repulsion of the impurity is finite, while at low temperature the negativity between the impurity spin and the bath exhibits the same power-law scaling behavior as in the Kondo model.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Quantum and electron transport phenomena · Quantum many-body systems · Quantum Information and Cryptography

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

References (47)

Show source-provided references
1. M. B. Plenio · Quantum Inf. Comput. · 2007 · 7 · 1
2. 10.1016/j.physrep.2009.02.00410.1016/j.physrep.2009.02.004 ↗
3. 10.1103/RevModPhys.81.86510.1103/RevModPhys.81.865 ↗
4. 10.1103/RevModPhys.80.51710.1103/RevModPhys.80.517 ↗
5. 10.1103/RevModPhys.82.27710.1103/RevModPhys.82.277 ↗
6. 10.1016/j.physrep.2016.06.00810.1016/j.physrep.2016.06.008 ↗
7. 10.1103/PhysRevLett.96.11040410.1103/PhysRevLett.96.110404 ↗
8. 10.1103/PhysRevLett.96.11040510.1103/PhysRevLett.96.110405 ↗
9. 10.1103/PhysRevLett.90.22790210.1103/PhysRevLett.90.227902 ↗
10. A. C. Hewson · 1997
11. 10.1103/PhysRevB.81.06442910.1103/PhysRevB.81.064429 ↗
12. 10.1103/PhysRevLett.109.06640310.1103/PhysRevLett.109.066403 ↗
13. 10.1038/ncomms478410.1038/ncomms4784 ↗
14. 10.1103/PhysRevLett.114.05720310.1103/PhysRevLett.114.057203 ↗
15. 10.1103/PhysRevB.93.08110610.1103/PhysRevB.93.081106 ↗
16. 10.1103/PhysRevLett.118.03610210.1103/PhysRevLett.118.036102 ↗
17. 10.1103/PhysRevLett.120.14680110.1103/PhysRevLett.120.146801 ↗
18. L. Gurvits · 2003
19. S. Gharibian · Quantum Inf. Comput. · 2010 · 10 · 343
20. 10.1103/PhysRevA.54.382410.1103/PhysRevA.54.3824 ↗
21. 10.1080/0950034000823513810.1080/09500340008235138 ↗
22. 10.1103/PhysRevA.65.03231410.1103/PhysRevA.65.032314 ↗
23. 10.1103/PhysRevLett.95.09050310.1103/PhysRevLett.95.090503 ↗
24. 10.1103/PhysRevLett.80.523910.1103/PhysRevLett.80.5239 ↗
25. 10.1103/PhysRevA.66.04232710.1103/PhysRevA.66.042327 ↗
26. 10.1103/PhysRevA.77.06210210.1103/PhysRevA.77.062102 ↗
27. 10.1088/1367-2630/16/12/12302010.1088/1367-2630/16/12/123020 ↗
28. 10.1088/1367-2630/17/5/05304810.1088/1367-2630/17/5/053048 ↗
29. 10.1088/1751-8113/48/1/01500610.1088/1751-8113/48/1/015006 ↗
30. 10.1103/PhysRevE.93.02212810.1103/PhysRevE.93.022128 ↗
31. 10.1103/PhysRevLett.119.21050110.1103/PhysRevLett.119.210501 ↗
32. I. Affleck · 2010
33. 10.1103/PhysRevLett.110.24660310.1103/PhysRevLett.110.246603 ↗
34. 10.1103/RevModPhys.47.77310.1103/RevModPhys.47.773 ↗
35. 10.1103/RevModPhys.80.39510.1103/RevModPhys.80.395 ↗
36. 10.1103/PhysRevB.74.24511410.1103/PhysRevB.74.245114 ↗
37. 10.1103/PhysRevLett.99.07640210.1103/PhysRevLett.99.076402 ↗
38. 10.1103/PhysRevB.86.24512410.1103/PhysRevB.86.245124 ↗
39. 10.1126/science.116734310.1126/science.1167343 ↗
40. 10.1103/PhysRevLett.95.19680110.1103/PhysRevLett.95.196801 ↗
41. 10.1103/PhysRevB.49.1198610.1103/PhysRevB.49.11986 ↗
42. 10.1103/PhysRevB.72.10443210.1103/PhysRevB.72.104432 ↗
43. 10.1103/PhysRevB.78.24510910.1103/PhysRevB.78.245109 ↗
44. 10.1016/j.aop.2012.07.00910.1016/j.aop.2012.07.009 ↗
45. 10.1103/PhysRevB.86.07515310.1103/PhysRevB.86.075153 ↗
46. 10.1103/PhysRevB.61.691810.1103/PhysRevB.61.6918 ↗
47. 10.1103/PhysRevLett.80.224510.1103/PhysRevLett.80.2245 ↗