Loading…
Effect of Dzialoshinski–Moriya interaction on the quantum discord of a spin-star model
The effect of Dzialoshinski–Moriya (DM) interaction on the quantum discord and the thermal entanglement of the density matrix of a spin star model is investigated. Our results imply that the quantum correlation measured by quantum discord and thermal entanglement can be established between two surro...
Saved in:
Published in: | Physica A 2012-04, Vol.391 (7), p.2500-2506 |
---|---|
Main Authors: | , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Summary: | The effect of Dzialoshinski–Moriya (DM) interaction on the quantum discord and the thermal entanglement of the density matrix of a spin star model is investigated. Our results imply that the quantum correlation measured by quantum discord and thermal entanglement can be established between two surrounding parties both of which have no interaction with each other but interact with the central party independently. From the analysis, we find that the strong DM interaction can enhance the quantum discord and thermal entanglement while the external magnetic field with a large value and the high temperature can shrink them. Specially, the quantum discord is more robust than the thermal entanglement in the sense that the range of parameters in which the quantum discord takes a zero value is much smaller than that of the thermal entanglement.
► Effect of DM interaction on quantum discord of a spin star model is studied. ► Quantum discord and thermal entanglement of a spin star model are compared. ► Increasing DM interaction can enhance the quantum discord and thermal entanglement. ► Increasing the magnetic field and temperature will shrink the quantum correlation. ► Quantum discord can survive higher temperatures than the thermal entanglement does. |
---|---|
ISSN: | 0378-4371 1873-2119 |
DOI: | 10.1016/j.physa.2011.12.016 |