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Strong Subadditivity of Quantum Entropy : ウィキペディア英語版
Strong Subadditivity of Quantum Entropy
Strong subadditivity of entropy (SSA) was long known and appreciated in classical probability theory and
information theory.
Its extension to quantum mechanical entropy (the von Neumann entropy) was conjectured by D.W. Robinson and D. Ruelle 〔D. W. Robinson and D. Ruelle, Mean Entropy of States in Classical Statistical Mechanis, Communications in Mathematical Physics 5, 288 (1967)〕 in 1966 and O. E. Lanford III and D. W. Robinson 〔O. Lanford III, D. W. Robinson, Jour. Mathematical
Physics, 9, 1120 (1968)〕 in 1968 and proved
in 1973 by E.H. Lieb and M.B. Ruskai.〔E. H. Lieb, M. B. Ruskai, Proof of the Strong Subadditivity of Quantum Mechanichal Entropy, J. Math. Phys. 14, 1938–1941 (1973).〕 It is a basic theorem in modern quantum information theory.
SSA concerns the relation between the entropies of various subsystems of a larger system consisting of three subsystems (or of one system with three degrees of freedom). The proof of this relation in the classical case is quite easy
but the quantum case is difficult because of the non-commutativity of the density matrices describing
the subsystems.
Some useful references here are.〔M. Nielsen, I. Chuang Quantum Computation and Quantum Information, Cambr. U. Press, (2000)〕〔M. Ohya, D. Petz, Quantum Entropy and Its Use, Springer (1993)〕〔E. Carlen, Trace Inequalities and Quantum Entropy: An Introductory Course, Contemp. Math. 529 (2009).〕
==Definitions==

We will use the following notation throughout: A Hilbert space is denoted by \mathcal, and \mathcal(\mathcal) denotes the bounded linear operators on \mathcal.
Tensor products are denoted by superscripts, e.g., \mathcal^=\mathcal^1\otimes \mathcal^2. The trace
is denoted by .

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