Quantum Relative Entropy
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quantum information theory Quantum information is the information of the state of a quantum system. It is the basic entity of study in quantum information theory, and can be manipulated using quantum information processing techniques. Quantum information refers to both ...
, quantum relative entropy is a measure of distinguishability between two quantum states. It is the quantum mechanical analog of relative entropy.


Motivation

For simplicity, it will be assumed that all objects in the article are finite-dimensional. We first discuss the classical case. Suppose the probabilities of a finite sequence of events is given by the probability distribution ''P'' = , but somehow we mistakenly assumed it to be ''Q'' = . For instance, we can mistake an unfair coin for a fair one. According to this erroneous assumption, our uncertainty about the ''j''-th event, or equivalently, the amount of information provided after observing the ''j''-th event, is :\; - \log q_j. The (assumed) average uncertainty of all possible events is then :\; - \sum_j p_j \log q_j. On the other hand, the Shannon entropy of the probability distribution ''p'', defined by :\; - \sum_j p_j \log p_j, is the real amount of uncertainty before observation. Therefore the difference between these two quantities :\; - \sum_j p_j \log q_j - \left(- \sum_j p_j \log p_j\right) = \sum_j p_j \log p_j - \sum_j p_j \log q_j is a measure of the distinguishability of the two probability distributions ''p'' and ''q''. This is precisely the classical relative entropy, or
Kullback–Leibler divergence In mathematical statistics, the Kullback–Leibler divergence (also called relative entropy and I-divergence), denoted D_\text(P \parallel Q), is a type of statistical distance: a measure of how one probability distribution ''P'' is different fro ...
: :D_(P\, Q) = \sum_j p_j \log \frac \!. Note #In the definitions above, the convention that 0·log 0 = 0 is assumed, since \lim_ x \log(x) = 0. Intuitively, one would expect that an event of zero probability to contribute nothing towards entropy. #The relative entropy is not a metric. For example, it is not symmetric. The uncertainty discrepancy in mistaking a fair coin to be unfair is not the same as the opposite situation.


Definition

As with many other objects in quantum information theory, quantum relative entropy is defined by extending the classical definition from probability distributions to
density matrices In quantum mechanics, a density matrix (or density operator) is a matrix that describes the quantum state of a physical system. It allows for the calculation of the probabilities of the outcomes of any Measurement in quantum mechanics, measurement ...
. Let ''ρ'' be a density matrix. The von Neumann entropy of ''ρ'', which is the quantum mechanical analog of the Shannon entropy, is given by :S(\rho) = - \operatorname \rho \log \rho. For two density matrices ''ρ'' and ''σ'', the quantum relative entropy of ''ρ'' with respect to ''σ'' is defined by : S(\rho \, \sigma) = - \operatorname \rho \log \sigma - S(\rho) = \operatorname \rho \log \rho - \operatorname \rho \log \sigma = \operatorname\rho (\log \rho - \log \sigma). We see that, when the states are classically related, i.e. ''ρσ'' = ''σρ'', the definition coincides with the classical case, in the sense that if \rho = S D_1 S^ and \sigma = S D_2 S^ with D_1 = \text(\lambda_1, \ldots, \lambda_n) and D_2 = \text(\mu_1, \ldots, \mu_n) (because \rho and \sigma commute, they are
simultaneously diagonalizable In linear algebra, a square matrix A is called diagonalizable or non-defective if it is similar to a diagonal matrix, i.e., if there exists an invertible matrix P and a diagonal matrix D such that or equivalently (Such D are not unique.) ...
), then S(\rho \, \sigma) = \sum_^ \lambda_j \ln\left(\frac\right) is just the ordinary Kullback-Leibler divergence of the probability vector (\lambda_1, \ldots, \lambda_n) with respect to the probability vector (\mu_1, \ldots, \mu_n).


Non-finite (divergent) relative entropy

In general, the ''support'' of a matrix ''M'' is the orthogonal complement of its
kernel Kernel may refer to: Computing * Kernel (operating system), the central component of most operating systems * Kernel (image processing), a matrix used for image convolution * Compute kernel, in GPGPU programming * Kernel method, in machine lea ...
, i.e. \text(M) = \text(M)^\perp . When considering the quantum relative entropy, we assume the convention that −''s'' · log 0 = ∞ for any ''s'' > 0. This leads to the definition that :S(\rho \, \sigma) = \infty when :\text(\rho) \cap \text(\sigma) \neq \. This can be interpreted in the following way. Informally, the quantum relative entropy is a measure of our ability to distinguish two quantum states where larger values indicate states that are more different. Being orthogonal represents the most different quantum states can be. This is reflected by non-finite quantum relative entropy for orthogonal quantum states. Following the argument given in the Motivation section, if we erroneously assume the state \rho has support in \text(\sigma), this is an error impossible to recover from. However, one should be careful not to conclude that the divergence of the quantum relative entropy S(\rho\, \sigma) implies that the states \rho and \sigma are orthogonal or even very different by other measures. Specifically, S(\rho\, \sigma) can diverge when \rho and \sigma differ by a ''vanishingly small amount'' as measured by some norm. For example, let \sigma have the diagonal representation \sigma=\sum_\lambda_n, f_n\rangle\langle f_n, with \lambda_n>0 for n=0,1,2,\ldots and \lambda_n=0 for n=-1,-2,\ldots where \ is an orthonormal set. The kernel of \sigma is the space spanned by the set \. Next let \rho=\sigma+\epsilon, f_\rangle\langle f_, - \epsilon, f_1\rangle\langle f_1, for a small positive number \epsilon. As \rho has support (namely the state , f_\rangle) in the kernel of \sigma, S(\rho\, \sigma) is divergent even though the trace norm of the difference (\rho-\sigma) is 2\epsilon . This means that difference between \rho and \sigma as measured by the trace norm is vanishingly small as \epsilon\to 0 even though S(\rho\, \sigma) is divergent (i.e. infinite). This property of the quantum relative entropy represents a serious shortcoming if not treated with care.


Non-negativity of relative entropy


Corresponding classical statement

For the classical
Kullback–Leibler divergence In mathematical statistics, the Kullback–Leibler divergence (also called relative entropy and I-divergence), denoted D_\text(P \parallel Q), is a type of statistical distance: a measure of how one probability distribution ''P'' is different fro ...
, it can be shown that :D_(P\, Q) = \sum_j p_j \log \frac \geq 0, and the equality holds if and only if ''P'' = ''Q''. Colloquially, this means that the uncertainty calculated using erroneous assumptions is always greater than the real amount of uncertainty. To show the inequality, we rewrite :D_(P\, Q) = \sum_j p_j \log \frac = \sum_j (- \log \frac)(p_j). Notice that log is a concave function. Therefore -log is
convex Convex or convexity may refer to: Science and technology * Convex lens, in optics Mathematics * Convex set, containing the whole line segment that joins points ** Convex polygon, a polygon which encloses a convex set of points ** Convex polytop ...
. Applying Jensen's inequality, we obtain : D_(P\, Q) = \sum_j (- \log \frac)(p_j) \geq - \log ( \sum_j \frac p_j ) = 0. Jensen's inequality also states that equality holds if and only if, for all ''i'', ''qi'' = (Σ''qj'') ''pi'', i.e. ''p'' = ''q''.


The result

Klein's inequality states that the quantum relative entropy : S(\rho \, \sigma) = \operatorname\rho (\log \rho - \log \sigma). is non-negative in general. It is zero if and only if ''ρ'' = ''σ''. Proof Let ''ρ'' and ''σ'' have spectral decompositions :\rho = \sum_i p_i v_i v_i ^* \; , \; \sigma = \sum_i q_i w_i w_i ^*. So :\log \rho = \sum_i (\log p_i) v_i v_i ^* \; , \; \log \sigma = \sum_i (\log q_i)w_i w_i ^*. Direct calculation gives :S(\rho \, \sigma)= \sum_k p_k \log p_k - \sum_ (p_i \log q_j) , v_i ^* w_j , ^2 :\qquad \quad \; = \sum_i p_i ( \log p_i - \sum_j \log q_j , v_i ^* w_j , ^2) :\qquad \quad \; = \sum_i p_i (\log p_i - \sum_j (\log q_j )P_), where ''Pi j'' = , ''vi*wj'', 2. Since the matrix (''Pi j'')''i j'' is a doubly stochastic matrix and -log is a convex function, the above expression is :\geq \sum_i p_i (\log p_i - \log (\sum_j q_j P_)). Define ''r''i = Σ''j''''qj Pi j''. Then is a probability distribution. From the non-negativity of classical relative entropy, we have :S(\rho \, \sigma) \geq \sum_i p_i \log \frac \geq 0. The second part of the claim follows from the fact that, since -log is strictly convex, equality is achieved in : \sum_i p_i (\log p_i - \sum_j (\log q_j )P_) \geq \sum_i p_i (\log p_i - \log (\sum_j q_j P_)) if and only if (''Pi j'') is a permutation matrix, which implies ''ρ'' = ''σ'', after a suitable labeling of the eigenvectors and .


Joint convexity of relative entropy

The relative entropy is jointly convex. For 0\leq \lambda\leq 1 and states \rho_, \sigma_ we have D(\lambda\rho_1+(1-\lambda)\rho_2\, \lambda\sigma_1+(1-\lambda)\sigma_2)\leq \lambda D(\rho_1\, \sigma_1)+(1-\lambda)D(\rho_2\, \sigma_2)


Monotonicity of relative entropy

The relative entropy decreases monotonically under completely positive trace preserving (CPTP) operations \mathcal on density matrices, S(\mathcal(\rho)\, \mathcal(\sigma))\leq S(\rho\, \sigma). This inequality is called Monotonicity of quantum relative entropy and was first proved by Lindblad.


An entanglement measure

Let a composite quantum system have state space :H = \otimes _k H_k and ''ρ'' be a density matrix acting on ''H''. The relative entropy of entanglement of ''ρ'' is defined by :\; D_ (\rho) = \min_ S(\rho \, \sigma) where the minimum is taken over the family of separable states. A physical interpretation of the quantity is the optimal distinguishability of the state ''ρ'' from separable states. Clearly, when ''ρ'' is not entangled :\; D_ (\rho) = 0 by Klein's inequality.


Relation to other quantum information quantities

One reason the quantum relative entropy is useful is that several other important quantum information quantities are special cases of it. Often, theorems are stated in terms of the quantum relative entropy, which lead to immediate corollaries concerning the other quantities. Below, we list some of these relations. Let ''ρ''AB be the joint state of a bipartite system with subsystem ''A'' of dimension ''n''A and ''B'' of dimension ''n''B. Let ''ρ''A, ''ρ''B be the respective reduced states, and ''I''A, ''I''B the respective identities. The maximally mixed states are ''I''A/''n''A and ''I''B/''n''B. Then it is possible to show with direct computation that :S(\rho_ , , I_/n_A) = \mathrm(n_A)- S(\rho_), \; :S(\rho_ , , \rho_ \otimes \rho_) = S(\rho_) + S(\rho_) - S(\rho_) = I(A:B), :S(\rho_ , , \rho_ \otimes I_/n_B) = \mathrm(n_B) + S(\rho_) - S(\rho_) = \mathrm(n_B)- S(B, A), where ''I''(''A'':''B'') is the quantum mutual information and ''S''(''B'', ''A'') is the quantum conditional entropy.


References

* {{cite journal , last=Vedral , first=V. , title=The role of relative entropy in quantum information theory , journal=Reviews of Modern Physics , publisher=American Physical Society (APS) , volume=74 , issue=1 , date=8 March 2002 , issn=0034-6861 , doi=10.1103/revmodphys.74.197 , pages=197–234, arxiv=quant-ph/0102094, bibcode=2002RvMP...74..197V , s2cid=6370982 * Michael A. Nielsen, Isaac L. Chuang
"Quantum Computation and Quantum Information"
* Marco Tomamichel,
Quantum Information Processing with Finite Resources -- Mathematical Foundations
. arXiv:1504.00233 Quantum mechanical entropy Quantum information theory