Quantifying entanglement with witness operators
Creators
- 1. Grupo de Informacao Quantica, Departamento de Fisica, Universidade Federal de Minas Gerais, Caixa Postal 702, Belo Horizonte, 30.123-970, MG (Brazil)
Description
We present a unifying approach to the quantification of entanglement based on entanglement witnesses, which includes several already established entanglement measures such as the negativity, the concurrence, and the robustness of entanglement. We then introduce an infinite family of new entanglement quantifiers, having as its limits the best separable approximation measure and the generalized robustness. Gaussian states, states with symmetry, states constrained to super-selection rules, and states composed of indistinguishable particles are studied under the view of the witnessed entanglement. We derive new bounds to the fidelity of teleportation dmin, for the distillable entanglement ED and for the entanglement of formation. A particular measure, the PPT-generalized robustness, stands out due to its easy calculability and provides sharper bounds to dmin and ED than the negativity in most of the states. We illustrate our approach studying thermodynamical properties of entanglement in the Heisenberg XXX and dimerized models
Additional details
Identifiers
- DOI
- 10.1103/PhysRevA.72.022310;
- arXiv
- arXiv:quant-ph/0503152v10;
Publishing Information
- Journal Title
- Physical Review. A
- Journal Volume
- 72
- Journal Issue
- 2
- Journal Page Range
- p. 022310-022310.15
- ISSN
- 1050-2947
- CODEN
- PLRAAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37030332
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- HEISENBERG MODEL; INFORMATION THEORY; QUANTUM ENTANGLEMENT; QUANTUM TELEPORTATION; SELECTION RULES; SYMMETRY; THERMODYNAMIC PROPERTIES
- Descriptors DEC
- CRYSTAL MODELS; MATHEMATICAL MODELS; PHYSICAL PROPERTIES
Optional Information
- Notes
- (c) 2005 The American Physical Society