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Optimizing entanglement in two-qubit systems

Salvio Luna-Hernández Claudia Quintana Oscar Rosas-Ortiz
Abstract

We investigate entanglement in two-qubit systems using a geometric representation based on the minimum of essential parameters. The latter is achieved by requiring subsystems with the same entropy, regardless of whether the state of the entire system is pure or mixed. The geometric framework is provided by a convex set 𝒮\mathcal{S} that forms a right-triangle, whose points are linked to just two of the coherences of the system under study. As a result, we find that optimized states of two qubits are X–shaped and host pairs of identical populations while reducing the number of coherences involved. A geometric LL-measure of entanglement is introduced as the distance between the points in 𝒮\mathcal{S} that represent entangled states and the closest point that defines separable states. It is shown that LL reproduces the results of the Hill-Wootters concurrence CC, so that CC can be interpreted as a distance-like entanglement measure. However, unlike CC, the measure LL also distinguishes the rank of states. The universality of the two-qubit X–states ensures the utility of our geometric model for studying entanglement of two-qubit states in any configuration. To show the applicability of our approach far beyond time-independent cases, we construct a time-dependent two-qubit state, traced out over the complementary components of a pure tetra-partite system, and find that its one-qubit states share the same entropy. The entanglement measure results bounded from above by the envelope of the minima of such entropy.

1 Main

Quantum correlations characterize the features of quantum multipartite systems that cannot be described by classical–like theories. Closely related to the concept of quantum coherence, no quantum correlation is viable without interference with respect to distinguishable alternatives of quantum states. Nowadays nonclassical correlations are invaluable resources for quantum information and quantum computation [1], but they emerged on the scene by raising one of the most important problems in the foundations of quantum theory [2, 3] and, surprisingly, by providing the solution of the same [4, 5]. Schrödinger introduced the expression entanglement for this first manifestation of quantum correlation [3]. The concept describes what occurs with our knowledge of two systems that are separated after they were interacting for a while, and from which we had maximal knowledge before the interaction [6]. In this sense, entanglement implies that the state of a composite system cannot be separated into the states of its parts. However, entanglement does not account for all quantum correlations, and even separable states may exhibit correlations that are not completely classical.

The entanglement in a system can be characterized and quantified from different points of view [7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18]. However, the separability criterion introduced by Peres [19] and the Horodecki family [20] provides a powerful tool for its detection. In this work, the Peres-Horodecki (also known as positive partial transpose –PPT–) criterion is applied to construct a convex representation of two-qubit states that permits the study of entanglement in purely geometric form. It is well known that this criterion is necessary and sufficient to detect entanglement in 222\otimes 2 and 232\otimes 3 quantum systems [20], so we will use it to identify entanglement in two-qubit mixed states. There are several incentives to consider these states, mainly because generating pure entangled states is not an easy task, so entangled states could be prepared as statistical mixtures for purely experimental reasons, but in general they can be the result of a partial trace of the quantum state of a larger system.

In general, mixed states characterize the interaction between the system and its environment, and the study of their entanglement properties is not only more complicated than that of pure states, but lesser understood. Although the first entangled system found in physics was in a pure state [2], it is in one of the Bell states [4], shortly after mixed states were identified that also disrupt the foundations of quantum theory [21]. These states, named after Werner, can be modeled using hidden variables without violating the Bell inequalities, and find applications in a diversity of quantum entanglement subjects [22, 23, 24, 25, 26, 28, 27, 29, 30, 31]. Our results include a wide class of Werner states as a particular case.

We investigate the entanglement properties of two-qubit systems by using the minimum of essential parameters. The idea is to construct density operators whose reduced one-qubit states share the same entropy, regardless of whether the state of the entire system is pure or mixed. In this way, we identify X–shaped states [32, 33, 34, 35, 36, 37, 38], denoted ρX\rho_{X}, that have the capacity to host pairs of identical populations while reducing the number of coherences involved. The X–states played a significant role to show that nonlocal disentanglement times are shorter than local decoherence times for spontaneous emission of two initially entangled qubits [33] (see also [34]). One of the most relevant things to note is that concurrence takes a very simple form for X–states [35, 36, 37], which justifies the extensive application of these states to study the dynamics of entanglement between two qubits [33, 34, 35, 36, 37, 38, 39, 40, 41, 42, 43]. Demanding positive semidefinite, self-adjoint and normalized density operators ρX\rho_{X}, and imposing the Peres-Horodecki criterion, we arrive at the system of inequalities that related matrix elements must satisfy to determine both, the eligibility of ρX\rho_{X} as a quantum state, and the possibility of finding entanglement [37]. We show that the solution of such a system defines a convex set 𝒮\mathcal{S} that can be divided in subsets whose points are linked to separable states and regions where entanglement may be found.

Based on the convex representation provided by 𝒮\mathcal{S}, we introduce a geometric LL-measure of entanglement, a distance-like entanglement measure [44], that reproduces the results of the Hill-Wootters generalized concurrence CC [45, 46] when applied to states ρX\rho_{X}. Thus, our results give CC a geometric meaning that is not obvious without the convex structure 𝒮\mathcal{S}. However, unlike CC, the measure LL distinguishes the rank of states with maximum entanglement. The latter is relevant to determine not only the amount of quantum correlations but rather the quantumness of the state [47], so it shows how much useful a state is for a specific quantum processing task [48, 49]. Another advantage of the geometric LL-measure is that, with respect to other entanglement measures, it allows comparatively easy calculation.

The universality of two-qubit X–states was first explored numerically [50]. There, it is presented ‘strong numerical evidence showing that any general state can indeed be transformed to an X state of the same entanglement’. It has later been shown that X–states are in fact universal [38]. That is, given a two-qubit density operator ρ\rho, a unitary transformation can be found that produces an X–shaped state ρX\rho_{X} with equal (or higher) entanglement than ρ\rho. The spectrum and purity of ρ\rho are inherited unchanged to ρX\rho_{X}. In this way, the geometric formulation we develop throughout this work for two-qubit X–states is useful for any configuration of the two-qubit density operators.

We also study what happens to entanglement when the system depends explicitly on time. Modeling an entangled diatomic system whose one-qubit parts are placed in independent, isolated and identical electromagnetic cavities, each of which contains nn photons, we construct a tetra-partite pure state that continues to evolve unitarily as a pure state. However, the reduced diatomic state does not evolve in a reversible way (systems like this may show signatures of chaos [51]), which makes it an excellent subject of study to understand the behavior of entanglement in systems described by time-dependent statistical mixtures. Regardless of the dynamical law obeyed by the time-dependent diatomic state, the corresponding one-qubit states share the same von Neumann entropy SS, which oscillates as time passes. Our results verify that finding reduced states of maximum mixing does not provide information about the entanglement (if any) of the entire system when it is in a mixed state. However, the envelope formed by the minima of SS defines an upper bound for the entanglement measure. To the best of our knowledge, this remarkable result has gone unnoticed in the literature on the matter.

2 Two-qubit states

The density operator of any two-qubit system can be written as a 4×44\times 4 complex matrix over the field \mathbb{C},

ρ=(rkj),rjk=rkj,k,j{1,2,3,4},k=14rkk=1,\rho=\left(r_{kj}\right),\quad r_{jk}=r^{*}_{kj}\in\mathbb{C},\quad k,j\in\{1,2,3,4\},\quad\sum_{k=1}^{4}r_{kk}=1, (1)

where zz^{*} stands for the complex-conjugate of zz\in\mathbb{C}. The populations (diagonal elements) and coherences (off-diagonal elements) are such that ρ\rho is self-adjoint (ρ=ρ\rho=\rho^{\dagger}), normalized (Trρ=1\operatorname{Tr}\rho=1) and positive semidefinite (ρ0\rho\geq 0). The condition Trρ2=1\operatorname{Tr}\rho^{2}=1 is necessary and sufficient for a density operator ρ\rho to represent a pure state. In turn, ρ\rho refers to mixed states if Trρ2<1\operatorname{Tr}\rho^{2}<1. Thus, in general, matrix (1) is defined by 15 real parameters.

Hereafter, to represent states in the Hilbert space =4\mathcal{H}=\mathbb{C}^{4}, we use the computational basis |00|e1|00\rangle\equiv|e_{1}\rangle, |01|e2|01\rangle\equiv|e_{2}\rangle, |10|e3|10\rangle\equiv|e_{3}\rangle, |11|e4|11\rangle\equiv|e_{4}\rangle, with |e1=(1,0,0,0)T|e_{1}\rangle=(1,0,0,0)^{T}, and so on.

Assuming that the matrix-representation of ρ\rho is known in advance, there is a simple way to identify whether or not it represents a pure state, which consists of the applicability of the following proposition (the proof is provided in Appendix A).

Proposition Q. If the matrix-elements of the two-qubit density operator ρ=(rkj)\rho=\left(r_{kj}\right) can be factorized in the form rkj=αkαjr_{kj}=\alpha_{k}\alpha^{*}_{j}, with αk,αj\alpha_{k},\alpha_{j}\in\mathbb{C}, and k,j{1,2,3,4}k,j\in\{1,2,3,4\}, then ρ\rho represents the pure state |ψ=k=14αk|ek|\psi\rangle=\sum_{k=1}^{4}\alpha_{k}|e_{k}\rangle.

We are interested in density operators whose matrix-elements do not necessarily satisfy Proposition Q, which opens the possibility of investigating entanglement in two-qubit mixed states. Among the diverse ways to prepare such states, we pay attention to the representation generated by the computational basis.

To outline the profile of the states of our interest, let us consider the reduced density operators ρ1,2=Tr2,1ρ\rho_{1,2}=\operatorname{Tr}_{2,1}\rho. After diagonalizing, we obtain ρk,diag=diag(λk,1λk)\rho_{k,\operatorname{diag}}=\operatorname{diag}\left(\lambda_{k},1-\lambda_{k}\right), where λk=(114detρk)/2\lambda_{k}=(1-\sqrt{1-4\det\rho_{k}})/2 is the smallest eigenvalue of ρk\rho_{k}. The probability vectors λk=(λk,1λk)\vec{\lambda}_{k}=\left(\lambda_{k},1-\lambda_{k}\right) do not match in general since detρ2=detρ1+Δ\det\rho_{2}=\det\rho_{1}+\Delta, with

Δ=(r11r44)(r22r33)+|r13+r24|2|r12+r34|2.\Delta=(r_{11}-r_{44})(r_{22}-r_{33})+|r_{13}+r_{24}|^{2}-|r_{12}+r_{34}|^{2}. (2)

However, if Δ=0\Delta=0 then λ1=λ2=λ=(λ,1λ)\vec{\lambda}_{1}=\vec{\lambda}_{2}=\vec{\lambda}=(\lambda,1-\lambda) and ρ1,diag=ρ2,diag\rho_{1,\operatorname{diag}}=\rho_{2,\operatorname{diag}}. In such a case the von Neumann entropy gives the same result for both reduced matrices S(ρ1)=S(ρ2)S(\rho_{1})=S(\rho_{2}).

Throughout this work the search for subsystems with equal entropy serves as a way to construct two-qubit mixed states that require a reduced number of parameters to characterize their possible entanglement. As long as we have these states, we will establish a mechanism to identify (and measure) entanglement.

With respect to the degree of mixing, the matrix rank of ρ\rho (the number of its nonzero eigenvalues) is quite useful since it identifies the minimum number of pure states needed to prepare the corresponding statistical mixture. In fact, this notion is directly related to the purity of ρ\rho, 14η=Trρ21\tfrac{1}{4}\leq\eta=\operatorname{Tr}\rho^{2}\leq 1, since a pure state has rank 1 (and purity 1). So that purity less than 1 implies rank greater than 1. In this way, the maximally mixed state ρ=14𝕀\rho_{\star}=\tfrac{1}{4}\mathbb{I} has rank 4 (and purity 1/4).

A very simple form to satisfy Δ=0\Delta=0 is by imposing the constraint

r13=r24=r12=r34=0,r_{13}=r_{24}=r_{12}=r_{34}=0, (3)

which yields diagonal reduced matrices, together with at least one of the following conditions

r11=r44,r22=r33.r_{11}=r_{44},\quad r_{22}=r_{33}. (4)

Note that (3) removes 8 parameters from ρ\rho while (4) cancels at least one more parameter. In this way, as long as Δ=0\Delta=0 is true, a maximum of 6 real parameters will suffice to define the quantum states ρ\rho that we study below.

2.1 Optimized states of two qubits are X–shaped

To construct states that satisfy the Δ=0\Delta=0 requirement, let us first consider that only condition (3) is satisfied. In this case the density operators (1) require only 7 real parameters and are X–shaped,

ρX=(r1100r140r22r2300r23r330r1400r44).\rho_{X}=\left(\begin{array}[]{cccc}r_{11}&0&0&r_{14}\\ 0&r_{22}&r_{23}&0\\ 0&r_{23}^{*}&r_{33}&0\\ r_{14}^{*}&0&0&r_{44}\end{array}\right). (5)

Since coherence is a basis-dependent concept, states represented by non-diagonal density operators contain a certain amount of coherence with respect to the chosen basis. To be concrete, as density operators (1) are written in terms of the computational basis, their nonzero coherences rkjr_{kj}, kjk\neq j, determine the possibility of quantum interference with respect to the distinguishable alternatives |ek|e_{k}\rangle and |ej|e_{j}\rangle. In this way, for X–states (5), interference is only allowed between |e1=|00|e_{1}\rangle=|00\rangle and |e4=|11|e_{4}\rangle=|11\rangle, as well as between |e2=|01|e_{2}\rangle=|01\rangle and |e3=|10|e_{3}\rangle=|10\rangle. Any other interference between the elements of the basis is not allowed. In the most general case both interferences occur simultaneously, but entanglement arises when at least one of them is activated.

To analyze the properties of X–states as generally as possible, it is necessary to ensure that ρX\rho_{X} is in fact a density operator. By construction, ρX\rho_{X} is self-adjoint and normalized, so we just need to make sure that it is positive semidefinite.

After calculating the eigenvalues of ρX\rho_{X}, see explicit expressions in Eq. (A-1) of Appendix A, we find that they are non-negative as long as the following conditions are met [37]:

|r14|r11r44,|r23|r22r33.|r_{14}|\leq\sqrt{r_{11}r_{44}},\qquad|r_{23}|\leq\sqrt{r_{22}r_{33}}. (6)

That is, ρX\rho_{X} represents an admissible quantum state, pure or mixed, only if the coherence amplitudes |r14||r_{14}| and |r23||r_{23}| are upper bounded by the population of the corresponding states. Note that the phases of r14r_{14} and r23r_{23} play no role in characterizing ρX\rho_{X} as a positive semidefinite matrix. Nevertheless, they characterize quantum interference with respect to the corresponding distinguishable alternatives.

2.1.1 Subsystems with equal entropy

Assuming that not only (3) but the first identity of Eq. (4) is also satisfied, states (5) will have the same population for states |e1=|00|e_{1}\rangle=|00\rangle and |e4=|11|e_{4}\rangle=|11\rangle. As a consequence, the reduced states will have the same probability vector λL=(λL,1λL)\vec{\lambda}_{L}=(\lambda_{L},1-\lambda_{L}), with λL=(1|r22r33|)/2\lambda_{L}=(1-|r_{22}-r_{33}|)/2 and 2r11+r22+r33=12r_{11}+r_{22}+r_{33}=1.

On the other hand, satisfying (3) and the second identity of Eq. (4) leads to states (5) characterized by having the same population for states |e2=|01|e_{2}\rangle=|01\rangle and |e3=|10|e_{3}\rangle=|10\rangle. The probability vector is now λR=(λR,1λR)\vec{\lambda}_{R}=(\lambda_{R},1-\lambda_{R}), with λR=(1|r11r44|)/2\lambda_{R}=(1-|r_{11}-r_{44}|)/2 and r11+2r22+r44=1r_{11}+2r_{22}+r_{44}=1.

Since populations satisfy 0rkk10\leq r_{kk}\leq 1, we obtain 0λL,R120\leq\lambda_{L,R}\leq\frac{1}{2}. That is, in general, neither of the two previous cases maximizes entropy.

Reduced matrices with maximal entropy are achieved if, in addition, we make r22=r33r_{22}=r_{33} in λL\lambda_{L} and r11=r44r_{11}=r_{44} in λR\lambda_{R}. The latter corresponds to also satisfying the complementary identity of Eq. (4) in each case. That is, only if (3) and both identities of (4) are satisfied, one gets λL=λR=1/2\lambda_{L}=\lambda_{R}=1/2.

The above reasoning applies to ρX\rho_{X} matrices regardless of whether they represent pure or mixed states. Therefore, when (3) and both identities in (4) hold, the density operators (5) are optimized and host pairs of identical populations. This further reduces the number of parameters needed to define ρX\rho_{X} from 7 to just 5.

With respect to the pure states represented by the optimized ρX\rho_{X} matrices, in Appendix A we show that once Proposition Q is satisfied, when (3) and both identities of (4) hold, we recover the Bell–states

|β1=|e1+|e42,|β2=|e1|e42,|\beta_{1}\rangle=\frac{|e_{1}\rangle+|e_{4}\rangle}{\sqrt{2}},\qquad|\beta_{2}\rangle=\frac{|e_{1}\rangle-|e_{4}\rangle}{\sqrt{2}}, (7)

and

|β3=|e2+|e32,|β4=|e2|e32.|\beta_{3}\rangle=\frac{|e_{2}\rangle+|e_{3}\rangle}{\sqrt{2}},\qquad|\beta_{4}\rangle=\frac{|e_{2}\rangle-|e_{3}\rangle}{\sqrt{2}}. (8)

So the Bell basis elements (7)-(8) are optimized states of two qubits.

To give a more general example, consider the convex combinations

ρB=k=14bk|βkβk|,0bk1,k=14bk=1.\rho_{B}=\sum_{k=1}^{4}b_{k}|\beta_{k}\rangle\langle\beta_{k}|,\quad 0\leq b_{k}\leq 1,\quad\sum_{k=1}^{4}b_{k}=1. (9)

This family of density operators is not only X–shaped; their members accommodate two pairs of equally weighted populations and reduce the number of coherences. Namely, the density operators ρB\rho_{B} are optimized:

ρB=12(b1+b200b1b20b3+b4b3b400b3b4b3+b40b1b200b1+b2).\rho_{B}=\frac{1}{2}\left(\begin{array}[]{cccc}b_{1}+b_{2}&0&0&b_{1}-b_{2}\\ 0&b_{3}+b_{4}&b_{3}-b_{4}&0\\ 0&b_{3}-b_{4}&b_{3}+b_{4}&0\\ b_{1}-b_{2}&0&0&b_{1}+b_{2}\end{array}\right). (10)

The one-qubit states that make up any state ρB\rho_{B} are maximally mixed S(ρB,1)=S(ρB,2)=1S(\rho_{B,1})=S(\rho_{B,2})=1. This set of optimized two-qubit states includes two special configurations, the first reduces ρB\rho_{B} to a single Bell–state (bk=1b_{k}=1 for a given kk), ρB=|βkβk|\rho_{B}=|\beta_{k}\rangle\langle\beta_{k}|, and the second yields an equally weighted statistical mixture of Bell–states (bk=14b_{k}=\frac{1}{4} for any kk), ρB=ρ\rho_{B}=\rho_{\star}.

For states ρB\rho_{B}, the coherences r14=r14=b1b2r_{14}=r_{14}^{*}=b_{1}-b_{2} and r23=r23=b3b4r_{23}=r_{23}^{*}=b_{3}-b_{4} are activated whenever b1b2b_{1}\neq b_{2} and b3b4b_{3}\neq b_{4}, respectively. This property allows us to identify other interesting cases of optimized two-qubit states. For example, interference between |e2=|01|e_{2}\rangle=|01\rangle and |e3=|10|e_{3}\rangle=|10\rangle is not allowed if r23=0r_{23}=0, which can be achieved by setting b3=b4=κb_{3}=b_{4}=\kappa in (9) to get

ρB|b3=b4=κ=b1|β1β1|+b2|β2β2|+κ(|0101|+|1010|),b1+b2+2κ=1.\left.\rho_{B}\right|_{b_{3}=b_{4}=\kappa}=b_{1}|\beta_{1}\rangle\langle\beta_{1}|+b_{2}|\beta_{2}\rangle\langle\beta_{2}|+\kappa\left(|01\rangle\langle 01|+|10\rangle\langle 10|\right),\quad b_{1}+b_{2}+2\kappa=1. (11)

To avoid reaching a statistical mixture of the computational basis, we will require b1b2b_{1}\neq b_{2}. The matrix representation is easily obtained from (10) and reads as follows

ρB|b3=b4=κ=(b1+b2200b1b220κ0000κ0b1b2200b1+b22),b1b2,b1+b2+2κ=1.\left.\rho_{B}\right|_{b_{3}=b_{4}=\kappa}=\left(\begin{array}[]{cccc}\frac{b_{1}+b_{2}}{2}&0&0&\frac{b_{1}-b_{2}}{2}\\ 0&\kappa&0&0\\ 0&0&\kappa&0\\ \frac{b_{1}-b_{2}}{2}&0&0&\frac{b_{1}+b_{2}}{2}\end{array}\right),\quad b_{1}\neq b_{2},\quad b_{1}+b_{2}+2\kappa=1. (12)

As we can see, what distinguishes this state from a statistical mixture of the basis elements is the coherence value r14=(b1b2)/2r_{14}=(b_{1}-b_{2})/2. The greater the interference between |e1=|00|e_{1}\rangle=|00\rangle and |e4=|11|e_{4}\rangle=|11\rangle, the greater the difference.

An important case of the previous model is achieved by setting bk=(1+3q)/4b_{k}=(1+3q)/4, and bj=(1q)/4b_{j}=(1-q)/4 for k=fixedk=\operatorname{fixed}, and jkj\neq k. This leads to the Werner–states [21]:

ρWk=q|βkβk|+(1q4)𝕀,13q1,k=1,2,3,4.\rho_{W_{k}}=q|\beta_{k}\rangle\langle\beta_{k}|+\left(\tfrac{1-q}{4}\right)\mathbb{I},\quad-\tfrac{1}{3}\leq q\leq 1,\quad k=1,2,3,4. (13)

Explicitly,

ρWj=(1+q400()j+1q201q400001q40()j+1q2001+q4),ρW=(1q400001+q4()1q200()1q21+q400001q4),\displaystyle\rho_{W_{j}}=\left(\begin{array}[]{cccc}\frac{1+q}{4}&0&0&\frac{(-)^{j+1}q}{2}\\ 0&\frac{1-q}{4}&0&0\\ 0&0&\frac{1-q}{4}&0\\ \frac{(-)^{j+1}q}{2}&0&0&\frac{1+q}{4}\end{array}\right),\quad\rho_{W_{\ell}}=\left(\begin{array}[]{cccc}\frac{1-q}{4}&0&0&0\\ 0&\frac{1+q}{4}&\frac{(-)^{\ell-1}q}{2}&0\\[3.44444pt] 0&\frac{(-)^{\ell-1}q}{2}&\frac{1+q}{4}&0\\[3.44444pt] 0&0&0&\frac{1-q}{4}\end{array}\right), (22)

where j=1,2j=1,2 and =3,4\ell=3,4. That is, the Werner–states (22) are not only X–shaped but they are also optimized in the sense discussed above.

Comparing (22) with (12), we see that ρB|b3=b4=κ\left.\rho_{B}\right|_{b_{3}=b_{4}=\kappa} has the structure of the Werner–states ρWj\rho_{W_{j}}.

The Werner–states ρWk\rho_{W_{k}} can be generalized to the configuration

ρS=k=14qk|βkβk|+(1s4)𝕀,k=14qk=s,s14qks+34,\rho_{S}=\sum_{k=1}^{4}q_{k}|\beta_{k}\rangle\langle\beta_{k}|+\left(\tfrac{1-s}{4}\right)\mathbb{I},\quad\sum_{k=1}^{4}q_{k}=s,\quad\tfrac{s-1}{4}\leq q_{k}\leq\tfrac{s+3}{4}, (23)

where s1+qmins\leq 1+q_{\min} and qmin=min{q1,q2,q3,q4}q_{\min}=\min\{q_{1},q_{2},q_{3},q_{4}\}. The explicit form of these optimized density operators is as follows

ρS=(ϱ1100q1q220ϱ22q3q4200q3q42ϱ220q1q2200ϱ11),\rho_{S}=\left(\begin{array}[]{cccc}\varrho_{11}&0&0&\frac{q_{1}-q_{2}}{2}\\ 0&\varrho_{22}&\frac{q_{3}-q_{4}}{2}&0\\ 0&\frac{q_{3}-q_{4}}{2}&\varrho_{22}&0\\ \frac{q_{1}-q_{2}}{2}&0&0&\varrho_{11}\end{array}\right), (24)

where

ϱ11=14(1+q1+q2q3q4),ϱ22=14(1q1q2+q3+q4).\varrho_{11}=\tfrac{1}{4}\left(1+q_{1}+q_{2}-q_{3}-q_{4}\right),\qquad\varrho_{22}=\tfrac{1}{4}\left(1-q_{1}-q_{2}+q_{3}+q_{4}\right).

2.2 Entanglement conditions

The positive partial transposition of the density operator (1) obeys the following transformation rules

ρT1:r13r13,r14r23,r24r24.ρT2:r12r12,r14r23,r34r34.\begin{array}[]{c}\rho^{T_{1}}:\quad r_{13}\rightarrow r_{13}^{*},\,r_{14}\rightarrow r_{23}^{*},\,r_{24}\rightarrow r_{24}^{*}.\\[6.88889pt] \rho^{T_{2}}:\quad r_{12}\rightarrow r_{12}^{*},\,r_{14}\rightarrow r_{23},\,r_{34}\rightarrow r_{34}^{*}.\end{array}

Without loss of generality, we will use the transposition with respect to the second qubit.

The transposition of the X–state (5) corresponds to make r14r23r_{14}\rightarrow r_{23}. Eigenvalues (A-1) and eigenvectors (A-2) must be transformed accordingly to solve the eigenvalue equation ρXT2|ϵ~=Λ~|ϵ~\rho_{X}^{T_{2}}|\widetilde{\epsilon}\,\rangle=\widetilde{\Lambda}|\widetilde{\epsilon}\,\rangle. Then, it is found that ρXT2\rho_{X}^{T_{2}} is positive semidefinite whenever |r23|r11r44|r_{23}|\leq\sqrt{r_{11}r_{44}} and |r14|r22r33|r_{14}|\leq\sqrt{r_{22}r_{33}}. Applying the Peres–Horodecki criterion [19, 20], we find that ρX\rho_{X} is entangled as long as one of the following inequalities hold [37]:

|r23|>r11r44,|r14|>r22r33.|r_{23}|>\sqrt{r_{11}r_{44}},\qquad|r_{14}|>\sqrt{r_{22}r_{33}}. (25)

This result imposes a lower limit on the coherence amplitudes that is unexpectedly determined by the populations of the complementary states. That is, to find entanglement, |r14||r_{14}| must be lower bounded by the population of states |e2=|01|e_{2}\rangle=|01\rangle and |e3=|10|e_{3}\rangle=|10\rangle. Similar conclusions hold for the coherence amplitude |r23||r_{23}| and populations r11r_{11} and r44r_{44}.

Thus, once the populations of the X–states are known, the coherences determine both the eligibility of ρX\rho_{X} as a quantum state and the possibility of finding entanglement.

3 Convex optimization

To characterize entanglement in the X–states we have found a system of inequalities. Remember, (6) has been introduced to ensure that ρX\rho_{X} is positive semidefinite while (25) obeys the Peres–Horodecki criterion for entanglement.

Using shorter notation we write x0=r11r44x_{0}=\sqrt{r_{11}r_{44}}, y0=r22r33y_{0}=\sqrt{r_{22}r_{33}}, r14=xeiθr_{14}=xe^{i\theta} and r23=yeiϕr_{23}=ye^{i\phi}, with 0θ,ϕ<2π0\leq\theta,\phi<2\pi. In this way, condition (6) reads

0xx0,0yy0.0\leq x\leq x_{0},\quad 0\leq y\leq y_{0}. (26)

The combined inequalities (26) delimit a convex region of the xyxy–plane defined by 0x+yx0+y00\leq x+y\leq x_{0}+y_{0}. The maximum value of the upper bound is optimized as (x0+y0)max=1/2\left(x_{0}+y_{0}\right)_{\max}=1/2, see details in Appendix A. Therefore, ρX\rho_{X} is positive semidefinite for the points contained in the convex set

𝒮={(x,y)2;0x+y12}.\mathcal{S}=\left\{(x,y)\in\mathbb{R}^{2};0\leq x+y\leq\tfrac{1}{2}\right\}. (27)

Geometrically, 𝒮\mathcal{S} is nothing more than the right-triangle shown in Figure 1.

Refer to caption
Figure 1: The points of the convex set 𝒮2\mathcal{S}\subset\mathbb{R}^{2}, a right-triangle with legs of length 1/2, determine the matrix elements with which the density operator ρX\rho_{X} becomes positive semidefinite.

This is the scenario where at least one of the inequalities (25) must be satisfied to obtain entanglement. We have two possible configurations,

0yy0,y0<xx0,0\leq y\leq y_{0},\quad y_{0}<x\leq x_{0}, (28)

or

0xx0,x0<yy0.0\leq x\leq x_{0},\quad x_{0}<y\leq y_{0}. (29)

Consider for example the Werner–states (13). If k=1,2k=1,2, we find y=0y=0, x=12|q|x=\frac{1}{2}|q|, y0=14(1q)y_{0}=\frac{1}{4}(1-q) and x0=14(1+q)x_{0}=\frac{1}{4}(1+q), see Figure 2(a). To find entanglement, xx must obey inequalities (28). If k=3,4k=3,4, the results are obtained from the latter by changing x0y0x_{0}\leftrightarrow y_{0} and xyx\leftrightarrow y, see Figure 2(b). Entanglement is now found whenever yy obeys inequalities (29).

Refer to caption
(a) ρW1,2\rho_{W_{1,2}}
Refer to caption
(b) ρW3,4\rho_{W_{3,4}}
Figure 2: Entanglement conditions for the Werner–states ρWk\rho_{W_{k}}, with x=|r14|x=|r_{14}| (blue-continuous), y=|r23|y=|r_{23}| (red continuous), x0=r11r44x_{0}=\sqrt{r_{11}r_{44}} (blue-dotted), and y0=r22r33y_{0}=\sqrt{r_{22}r_{33}} (red-dashed). Two general cases are distinguished (a) If k=1,2k=1,2, then y=0y=0. To find entanglement the coherence amplitude xx must obey inequalities (28), see shaded-red area (b) If k=3,4k=3,4, then x=0x=0. Entanglement is found whenever the coherence amplitude yy obeys inequalities (29), see shaded-blue area.

The most striking thing about the above results is that all states ρWk\rho_{W_{k}} share the same entanglement profile: they are entangled for q(1/3,1]q\in(1/3,1], regardless of kk.

Note that ρWk\rho_{W_{k}} coincides with ρB\rho_{B} if bk=(3q+1)/4b_{k}=(3q+1)/4 and bj=(1q)/4b_{j}=(1-q)/4, where k=fixedk=\operatorname{fixed} and jkj\neq k. That is, the states ρWk\rho_{W_{k}} shown in Figure 2 correspond to concrete convex combinations of the four Bell–states, where |βk|\beta_{k}\rangle plays a leading role.

To highlight the relevance of the Bell–states involved in any statistical mixture, let us analyze the (generalized) Werner–state (23) with only two non-zero qkq_{k} coefficients. If s1s\neq 1, this state also involves the four Bell–states. However, if s=1s=1, it is reduced to a statistical mixture of only two Bell–states, those involved with coefficients qk0q_{k}\neq 0. The model is illustrated in Figure 3 with bk=qb_{k}=q, bj=1qb_{j}=1-q, and qk=qq_{k}=q, qj=sqq_{j}=s-q, for ρB\rho_{B} and ρS\rho_{S} respectively. In all cases kk and jkj\neq k are fixed. As in the previous case, what is common in all the states shown in Figure 3 is their entanglement profile.

Refer to caption
(a) ρB\rho_{B}, ρS\rho_{S}, s=1s=1
Refer to caption
(b) ρS\rho_{S}, s=3/4s=3/4
Refer to caption
(c) ρS\rho_{S}, s=1/2s=1/2
Refer to caption
(d) ρB\rho_{B}, ρS\rho_{S}, s=1s=1
Refer to caption
(e) ρS\rho_{S}, s=3/4s=3/4
Refer to caption
(f) ρS\rho_{S}, s=1/2s=1/2
Figure 3: Entanglement conditions for the statistical mixture of Bell–states ρB\rho_{B} and the generalized Werner–state ρS\rho_{S}, with only two nonzero coefficients bk=qb_{k}=q, bj=1qb_{j}=1-q, and qk=qq_{k}=q, qj=sqq_{j}=s-q, respectively. In all cases kk and jkj\neq k are fixed. The first row refers to any pair (k,j)(k,j), except (1,2)(1,2) and (3,4)(3,4). The second row illustrates the case (1,2)(1,2), for which y=0y=0. The case (3,4)(3,4) is obtained from the second row after the changes x0y0x_{0}\leftrightarrow y_{0}, xyx\leftrightarrow y. Color code follows the instructions in Figure 2.

3.1 Entanglement

In what follows we assume that x0x_{0} and y0y_{0} are known in advance. The description in terms of the point p=(x,y)𝒮p=(x,y)\in\mathcal{S} corresponds to determining the possible entanglement with respect to the coherences r14r_{14} and r23r_{23}.

The convex set 𝒮\mathcal{S} can be divided into regions (subsets) whose points define separable states and regions where entanglement may be found. We distinguish three main classes, described below.

\bullet Region 0\mathcal{M}_{0}. No entanglement is allowed if r11r44=r22r330r_{11}r_{44}=r_{22}r_{33}\neq 0. That is, none of inequalities (28)-(29) apply if x0=y00x_{0}=y_{0}\neq 0. Instead we have 0x,yx00\leq x,y\leq x_{0}, so we arrive at a square x0\square_{x_{0}} of sides x0x_{0}, with x0max=1/4x_{0\max}=1/4, see Figure 4. These points produce separable mixed states ρX\rho_{X} that can be identified by their rank. According to the eigenvalues (A-1), the vertex q=(x0,x0)q_{\star}=(x_{0},x_{0}) represents rank-2 states. In turn, (x0,y)(x_{0},y) and (x,y0)(x,y_{0}), located respectively along the right-vertical and top sides of the square, define rank-3 states. Any other point of x0\square_{x_{0}} gives rank-4 states.

Refer to caption
Figure 4: There is no entanglement if the populations of ρX\rho_{X} satisfy r11r44=r22r330r_{11}r_{44}=r_{22}r_{33}\neq 0. In notation of the convex set 𝒮\mathcal{S}, the latter means x0=y00x_{0}=y_{0}\neq 0. The points (x,y)𝒮(x,y)\in\mathcal{S} that meet this condition form a square x0\square_{x_{0}} of sides x0x_{0}, with x0max=1/4x_{0\max}=1/4.

As an example consider the states ρB=ρS\rho_{B}=\rho_{S} shown in Figure 3(a). Entanglement is lost precisely at q=1/2q=1/2, where x0=y0=1/4x_{0}=y_{0}=1/4 puts vertex q=(x0,x0)q_{\star}=(x_{0},x_{0}) to the middle of the hypotenuse of 𝒮\mathcal{S}. The same is true for the states ρWk\rho_{W_{k}} exhibited in Figure 2, at q=0q=0.

\bullet Region 1\mathcal{M}_{1}. To satisfy inequalities (28) it is necessary to take the ordering 0y0<x00\leq y_{0}<x_{0}, see for example the shaded-red area in Figures 2 and 3. The entanglement set is a rectangle lying on the horizontal leg of 𝒮\mathcal{S}, as shown in Figure 5(a). The square y0\square_{y_{0}} of separable states is located just to the left of such rectangle.

Using the eigenvalues (A-1) we find that vertex q0=(x0,y0)q_{0}=(x_{0},y_{0}) gives rank-2 states. Points along the right-vertical side and the top of the rectangle, (x0,y)(x_{0},y) and (x,y0)(x,y_{0}) respectively, yield rank-3 states. Any other point of this entanglement set provides rank-4 states.

Refer to caption
(a) Region 1\mathcal{M}_{1}
Refer to caption
(b) r22=r33=0r_{22}=r_{33}=0
Figure 5: Entanglement conditions for states ρ1\rho_{\mathcal{M}_{1}}; the entanglement set is shaded-green, the chessboard region corresponds to separable states (a) According to (28), entanglement is encoded in a rectangle with base x0y0x_{0}-y_{0} and height y0y_{0}. The square y0\square_{y_{0}} defines separable states (b) Setting y=y0=0y=y_{0}=0, with r22=r33=0r_{22}=r_{33}=0, the states ρx\rho_{\mathcal{M}_{x}} acquire the form of the third matrix in Eq. (30), which is of rank-2 if x<x0x<x_{0}. The pure (rank-1) states |ψ14|\psi_{14}\rangle are achieved if x=x0x=x_{0}, which includes the Bell–states |β1,2|\beta_{1,2}\rangle when x=x0max=1/2x=x_{0\max}=1/2

A very important subset x1\mathcal{M}_{x}\subset\mathcal{M}_{1}, defined by the coherence amplitudes y=0y=0 (regardless of y0y_{0}), provides points restricted to the horizontal leg of 𝒮\mathcal{S}. Hereafter, the states defined by points (x,0)x(x,0)\in\mathcal{M}_{x} will be denoted by ρx\rho_{\mathcal{M}_{x}}. Since y=0y=0, to find entanglement, our interest is addressed to the coherence amplitudes xx that satisfy y0<xx0y_{0}<x\leq x_{0}. As an example consider the Werner–states ρW1,2\rho_{W_{1,2}} illustrated in Figure 2(a), as well as states ρS\rho_{S} shown in the second row of Figure 3.

In general, by extending the domain of xx to the maximum we optimize the entanglement in x\mathcal{M}_{x}. For this, it is enough to set y0=0y_{0}=0. We find three different sets of states

(r1100xeiθ000000r330xeiθ00r44),(r1100xeiθ0r22000000xeiθ00r44),(r1100xeiθ00000000xeiθ00r44).\left(\begin{array}[]{cccc}r_{11}&0&0&xe^{i\theta}\\ 0&0&0&0\\ 0&0&r_{33}&0\\ xe^{-i\theta}&0&0&r_{44}\end{array}\right),\quad\left(\begin{array}[]{cccc}r_{11}&0&0&xe^{i\theta}\\ 0&r_{22}&0&0\\ 0&0&0&0\\ xe^{-i\theta}&0&0&r_{44}\end{array}\right),\quad\left(\begin{array}[]{cccc}r_{11}&0&0&xe^{i\theta}\\ 0&0&0&0\\ 0&0&0&0\\ xe^{-i\theta}&0&0&r_{44}\end{array}\right). (30)

Neither of the first two matrices in (30) satisfy the factorization of their elements as required in Proposition Q, so they represent mixed states of rank-3 or rank-2, see Eq. (A-6). In turn, if the elements of the third matrix are factorized we have x=x0=|α1α4|x=x_{0}=|\alpha_{1}\alpha_{4}|, so it represents the pure (rank-1) state |ψ14|\psi_{14}\rangle defined in (A-3). In particular, if x=x0max=1/2x=x_{0\max}=1/2 we recover the Bell-states |β1|\beta_{1}\rangle and |β2|\beta_{2}\rangle. If their elements cannot be factorized, this matrix represents a mixed state of rank-2, see Figure 5(b).

Refer to caption
(a) Region 2\mathcal{M}_{2}
Refer to caption
(b) r11=r44=0r_{11}=r_{44}=0
Figure 6: Entanglement conditions for states ρ2\rho_{\mathcal{M}_{2}} (a) According to (29), we find entanglement in a rectangle of base x0x_{0} and height y0x0y_{0}-x_{0}. The square x0\square_{x_{0}} gives separable states (b) If x=x0=0x=x_{0}=0, with r11=r44=0r_{11}=r_{44}=0, the states ρy\rho_{\mathcal{M}_{y}} acquire the form of the third matrix in Eq. (31), which is of rank-2 if y<y0y<y_{0}. The pure (rank-1) states |ψ23|\psi_{23}\rangle are achieved if y=y0y=y_{0}, which includes the Bell–states |β3,4|\beta_{3,4}\rangle when y=y0max=1/2y=y_{0\max}=1/2.

\bullet Region 2\mathcal{M}_{2}. Inequalities (29) are satisfied by imposing the ordering 0x0<y00\leq x_{0}<y_{0}, see for example the shaded-blue area in Figures 2 and 3. The entanglement subset is also a rectangle, but in this case the base is placed just above the separable-states square x0\square_{x_{0}}, see Figure 6(a). Points along the right-vertical side and the top of the rectangle, respectively (x0,y)(x_{0},y) and (x,y0)(x,y_{0}), give rise to rank-3 states. In turn, vertex q0=(x0,y0)q_{0}=(x_{0},y_{0}) corresponds to rank-2 states. Any other point provides rank-4 states.

In this case the subset y2\mathcal{M}_{y}\subset\mathcal{M}_{2}, defined by the coherence amplitudes x=0x=0, provides points restricted to the vertical leg of 𝒮\mathcal{S} and defines states ρy\rho_{\mathcal{M}_{y}}. Our interest now turns to the region x0<yy0x_{0}<y\leq y_{0}. As an example consider the Werner–states ρW3,4\rho_{W_{3,4}} exhibited in Figure 2(b) and the yy-version of the states ρS\rho_{S} shown in the second row of Figure 3. The optimization is achieved by setting x0=0x_{0}=0, which results in the following states

(00000r22yeiϕ00yeiϕr330000r44),(r110000r22yeiϕ00yeiϕr3300000),(00000r22yeiϕ00yeiϕr3300000).\left(\begin{array}[]{cccc}0&0&0&0\\ 0&r_{22}&ye^{i\phi}&0\\ 0&ye^{-i\phi}&r_{33}&0\\ 0&0&0&r_{44}\end{array}\right),\quad\left(\begin{array}[]{cccc}r_{11}&0&0&0\\ 0&r_{22}&ye^{i\phi}&0\\ 0&ye^{-i\phi}&r_{33}&0\\ 0&0&0&0\end{array}\right),\quad\left(\begin{array}[]{cccc}0&0&0&0\\ 0&r_{22}&ye^{i\phi}&0\\ 0&ye^{-i\phi}&r_{33}&0\\ 0&0&0&0\end{array}\right). (31)

The first two matrices do not satisfy Proposition Q, so they represent mixed states of rank-3 or rank-2, see Eq. (A-7). If the elements of the third matrix are factorized we have y=y0=|α2α3|y=y_{0}=|\alpha_{2}\alpha_{3}|, so it represents the pure (rank-1) state |ψ23|\psi_{23}\rangle defined in (A-4). If y=y0max=1/2y=y_{0\max}=1/2, we recover the Bell-states |β3|\beta_{3}\rangle and |β4|\beta_{4}\rangle. If their elements cannot be factorized, this matrix is a mixed state of rank-2, see Figure 6(b).

The classification developed above is very close to the parametrization of two-qubit X–density matrices with a fixed rank reported in Section 2.1 of [38]. The latter, based on the coefficients that define the characteristic equation for the density operator, considers the Newton-Girard formulae [52] and a very concrete parametrization of the matrix-elements of ρX\rho_{X}. Beyond using the computational basis, our treatment is free of parametrization for the matrix elements rjkr_{jk}, so it aims to be more practical and, therefore, universal. Nevertheless, the parameters used in [38] are very valuable as they comprise the information needed to search for a unitary transformation that converts arbitrary two-qubit states into their X counterparts.

3.2 Geometric LL-measure

In the previous sections we have identified the regions of the convex set 𝒮\mathcal{S} whose points would imply entanglement in state ρX\rho_{X}. We know, for example, that squares x0\square_{x_{0}} and y0\square_{y_{0}} must be discarded because all their points represent separable states. However, we have not quantified the amount of entanglement that distinguishes some points from others in any other region, nor have we analyzed which region offers better entanglement conditions. To address these points we proceed as follows.

We seek to ensure that entangled states “resemble” separable states as little as possible. Translated into the language of the convex set 𝒮\mathcal{S}, this statement means that if pp encodes entanglement then it should be as far away as possible from x0\square_{x_{0}} and y0\square_{y_{0}}. The further remote, the greater the entanglement. With this in mind, consider the metric d(r1,r2)=max{|x2x1|,|y2y1|}d(\vec{r}_{1},\vec{r}_{2})=\max\{|x_{2}-x_{1}|,|y_{2}-y_{1}|\}, where rk=(xk,yk)2\vec{r}_{k}=(x_{k},y_{k})\in\mathbb{R}^{2}, k=1,2k=1,2. We now introduce a geometric measure of entanglement for two-qubit systems.

Definition. (LL-measure of entanglement) Given the extreme points x0x_{0} and y0y_{0}, let 𝒮\mathcal{S} be the convex set (27) and z0𝒮\square_{z_{0}}\subset\mathcal{S} be the subset of points defining separable states. The LL-measure of entanglement, applied to the point p𝒮p\in\mathcal{S}, is the distance between pp and the closest point qz0q\in\square_{z_{0}} given by

L=ξ0infqd(q,p),L=\xi_{0}\inf_{q}d(q,p),

with ξ0\xi_{0} a normalization factor.

Refer to caption
(a) Region 1\mathcal{M}_{1}
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(b) Region 2\mathcal{M}_{2}
Figure 7: Illustration of the geometric notion of distance used to define the measure LL for states ρX\rho_{X} defined by points in regions 1\mathcal{M}_{1} or 2\mathcal{M}_{2}.

Let us apply the measure LL to the points p𝒮p\in\mathcal{S} that define the states classified in the previous section.

States ρ1\rho_{\mathcal{M}_{1}} are such that infd(q,p)\inf d(q,p) is given by the points q=(y0,y)q=(y_{0},y), see Figure 7(a). Therefore

L(ρ1)|q=(y0,y)=2max{0,xy0}={0ifx<y02(xy0)ifx>y0\left.L(\rho_{\mathcal{M}_{1}})\right|_{q=(y_{0},y)}=2\max\left\{0,x-y_{0}\right\}=\left\{\begin{array}[]{cc}0&\operatorname{if}\,x<y_{0}\\[1.72221pt] 2(x-y_{0})&\operatorname{if}\,x>y_{0}\end{array}\right. (32)

Note that x=x0x=x_{0} defines the furthest point from the zone of separable states, therefore Lmax(ρ1)=2(x0y0)L_{\max}(\rho_{\mathcal{M}_{1}})=2(x_{0}-y_{0}). That is, among these states, the highest value of the LL-measure is provided by the rank-3 states associated with the points (x0,y)(x_{0},y).

For states ρ2\rho_{\mathcal{M}_{2}} we find that q=(x,x0)q=(x,x_{0}) defines infd(q,p)\inf d(q,p), see Figure 7(b). Then

L(ρ2)|q=(x,x0)=2max{0,yx0}={0ify<x02(yx0)ify>x0\left.L(\rho_{\mathcal{M}_{2}})\right|_{q=(x,x_{0})}=2\max\left\{0,y-x_{0}\right\}=\left\{\begin{array}[]{cc}0&\operatorname{if}\,y<x_{0}\\[1.72221pt] 2(y-x_{0})&\operatorname{if}\,y>x_{0}\end{array}\right. (33)

In this case the highest value of the LL-measure is provided by the rank-3 states associated with the points (x,y0)(x,y_{0}), so that Lmax(ρ2)=2(y0x0)L_{\max}(\rho_{\mathcal{M}_{2}})=2(y_{0}-x_{0}).

Combining the previous results we obtain the general rule

L(ρX)=2max{0,xy0,yx0}=2max{0,|r14|r22r33,|r23|r11r44}.\begin{array}[]{rl}L(\rho_{X})&=2\max\left\{0,x-y_{0},y-x_{0}\right\}\\[3.44444pt] &=2\max\left\{0,|r_{14}|-\sqrt{r_{22}r_{33}},\,|r_{23}|-\sqrt{r_{11}r_{44}}\,\right\}.\end{array} (34)

To find entanglement it is enough for one of the subtractions of (34) to be positive.

As for systems composed of subsystems with equal entropy, see Section 2.1.1, we have immediate results:

L(ρB)=2max{0,|b1b2|2(b3+b4)2,|b3b4|2(b1+b2)2},\displaystyle L(\rho_{B})=2\max\left\{0,\frac{|b_{1}-b_{2}|}{2}-\frac{(b_{3}+b_{4})}{2},\frac{|b_{3}-b_{4}|}{2}-\frac{(b_{1}+b_{2})}{2}\right\}, (35)
L(ρWk)=2max{0,|q|2|1q|4},\displaystyle L(\rho_{W_{k}})=2\max\left\{0,\frac{|q|}{2}-\frac{|1-q|}{4}\right\}, (36)
L(ρS)=2max{0,|q1q2|2ϱ22,|q3q4|2ϱ11}.\displaystyle L(\rho_{S})=2\max\left\{0,\frac{|q_{1}-q_{2}|}{2}-\varrho_{22},\frac{|q_{3}-q_{4}|}{2}-\varrho_{11}\right\}. (37)

To illustrate the applicability of the above expressions let us consider the state (11)-(12). From (35) one has

L(ρB)|b3=b4=κ=2max{0,|b1b2|2κ}.\left.L(\rho_{B})\right|_{b_{3}=b_{4}=\kappa}=2\max\left\{0,\frac{|b_{1}-b_{2}|}{2}-\kappa\right\}. (38)

Therefore, ρB|b3=b4=κ\left.\rho_{B}\right|_{b_{3}=b_{4}=\kappa} is disentangled if |b1b2|2κ=1(b1+b2)|b_{1}-b_{2}|\leq 2\kappa=1-(b_{1}+b_{2}). For these parameters the interference between |e1=|00|e_{1}\rangle=|00\rangle and |e4=|11|e_{4}\rangle=|11\rangle is so small that the system ends up behaving like a statistical mixture (a classical state) of the base states. On the other hand, for |b1b2|>2κ|b_{1}-b_{2}|>2\kappa we find entanglement with measure L(ρB)|b3=b4=κ=|b1b2|2κ\left.L(\rho_{B})\right|_{b_{3}=b_{4}=\kappa}=|b_{1}-b_{2}|-2\kappa . The extreme condition κ=0\kappa=0 shows that the statistical mixture of the Bell–states |β1|\beta_{1}\rangle and |β2|\beta_{2}\rangle is entangled, with a measure LL that is greater as the interference between |00|00\rangle and |11|11\rangle is more intense. In particular, setting b1=qb_{1}=q and b2=1qb_{2}=1-q we have L(ρB)|b3=b4=0=|2q1|\left.L(\rho_{B})\right|_{b_{3}=b_{4}=0}=|2q-1|. So state ρB|b3=b4=0\left.\rho_{B}\right|_{b_{3}=b_{4}=0} is disentangled for q=1/2q=1/2 (b1=b2b_{1}=b_{2}), as it is shown in Figures 3(a) and 3(d).

In general, if xx and yy take the maximum value in their respective domains we have

Lmax(ρX)=2max{0,x0y0,y0x0}=2|x0y0|=2|r11r44r22r33|.L_{\max}(\rho_{X})=2\max\left\{0,x_{0}-y_{0},y_{0}-x_{0}\right\}=2|x_{0}-y_{0}|=2\left|\sqrt{r_{11}r_{44}}-\sqrt{r_{22}r_{33}}\,\right|.

That is, when x0x_{0} and y0y_{0} are nonzero and different from each other, the strongest entanglement is exhibited by rank-3 states ρX\rho_{X}. On the other hand, if x0=0x_{0}=0 or y0=0y_{0}=0, the LL-measure identifies rank-1 (pure) states as those with greater entanglement. In particular, if x0=x0max=1/2x_{0}=x_{0\max}=1/2 or y0=y0max=1/2y_{0}=y_{0\max}=1/2, such states are not only pure but coincide with one of the Bell–states.

The most notable of the previous results is that the mathematical expression of the geometric measure LL coincides precisely with the Hill-Wootters concurrence calculated for the ρX\rho_{X} states [35, 36, 37]. In fact, according with [45, 46], the concurrence for any state ρ\rho is given by C(ρ)=max{0,1234}C(\rho)=\max\{0,\,\sqrt{\ell_{1}}-\sqrt{\ell_{2}}-\sqrt{\ell_{3}}-\sqrt{\ell_{4}}\}. The k\ell_{k}’s are the eigenvalues (in decreasing order) of the matrix Rρ=ρ(σ2σ2)ρ(σ2σ2)R_{\rho}=\rho\left(\sigma_{2}\otimes\sigma_{2}\right)\rho^{*}\left(\sigma_{2}\otimes\sigma_{2}\right), with σ2\sigma_{2} the well-known anti-diagonal Pauli-matrix.

Using state ρX\rho_{X} to construct RρR_{\rho}, a simple calculation produces the eigenvalues (x0±x)2(x_{0}\pm x)^{2} and (y0±y)2(y_{0}\pm y)^{2}, where no order has yet been established. From (26) we know that the quantities in parentheses are not negative, so we have two different ways of sorting k\sqrt{\ell_{k}} in descending order, with y0+yy_{0}+y or x0+xx_{0}+x leading. A little algebra produces the result

C(ρX)={2max{0,yx0},y0+y>x0+x2max{0,xy0},x0+x>y0+yC(\rho_{X})=\left\{\begin{array}[]{rl}2\max\left\{0,y-x_{0}\right\},&y_{0}+y>x_{0}+x\\[3.44444pt] 2\max\left\{0,x-y_{0}\right\},&x_{0}+x>y_{0}+y\end{array}\right.

which once summarized is written as follows [35, 36, 37]:

C(ρX)=2max{0,|r14|r22r33,|r23|r11r44}.C(\rho_{X})=2\max\left\{0,|r_{14}|-\sqrt{r_{22}r_{33}},\,|r_{23}|-\sqrt{r_{11}r_{44}}\,\right\}. (39)

Comparing (39) with (34) we find C(ρX)=L(ρX)C(\rho_{X})=L(\rho_{X}).

That is, the Hill-Wootters concurrence coincides with our LL-measure when applied to state ρX\rho_{X}. With this result we have given C(ρX)C(\rho_{X}) a geometric meaning that is not obvious without the structure of the convex set 𝒮\mathcal{S}. What is even better is that, unlike concurrence, the geometric measure distinguishes the rank of states with maximum entanglement.

In this context, the LL-measure of Werner–states (36) deserves special attention. First of all, this verifies that all states ρWk\rho_{W_{k}} share the same entanglement profile: they are entangled for q(1/3,1]q\in(1/3,1], regardless of kk, see Figure 2. On the other hand, two-qubit Werner–states can be prepared experimentally in such a way that the related hierarchy of quantum correlations can also be demonstrated. Indeed, in [27, 29], states (13) are prepared for various values of the mixing parameter qq, so that concurrence C(ρWk)=L(Wk)C(\rho_{W_{k}})=L({W_{k}}) is measured with good agreement of (36).

Once we have proven the identity C=LC=L, it is appropriate to construct a geometric version of the entanglement of formation [53]. Following [46] we obtain

ε(ρ1)={0ifx<y0h(1+14(xy0)22)ifx>y0\varepsilon(\rho_{\mathcal{M}_{1}})=\left\{\begin{array}[]{cc}0&\operatorname{if}\,x<y_{0}\\[1.72221pt] h\left(\frac{1+\sqrt{1-4(x-y_{0})^{2}}}{2}\right)&\operatorname{if}\,x>y_{0}\end{array}\right. (40)

and

ε(ρ2)={0ify<x0h(1+14(yx0)22)ify>x0\varepsilon(\rho_{\mathcal{M}_{2}})=\left\{\begin{array}[]{cc}0&\operatorname{if}\,y<x_{0}\\[1.72221pt] h\left(\frac{1+\sqrt{1-4(y-x_{0})^{2}}}{2}\right)&\operatorname{if}\,y>x_{0}\end{array}\right. (41)

where h(z)=zlog2z(1z)log2(1z)h(z)=-z\log_{2}z-(1-z)\log_{2}(1-z) is the Sahnnon binary entropy function.

3.3 Determination of entanglement

The entanglement of the Werner–states ρWk\rho_{W_{k}}, quantified by LL and ε\varepsilon, is shown in Figure 8(a) (see also Figure 2). The optimization is achieved in half of the domain of qq only. The experimental realization of Werner–states and the measurement of their entanglement can be found in [27, 29].

Refer to caption
(a) Werner states
Refer to caption
(b) Two-Bell mixed states
Figure 8: The geometric measure LL (dotted curve) and entanglement of formation ε\varepsilon (continuous curve) applied to (a) the Werner–states ρWk\rho_{W_{k}} and (b) the statistical mixture ρB\rho_{B} of only two Bell–states. There is no entanglement for half the domain of qq in ρWk\rho_{W_{k}}, compare with Figure 2. In turn, states ρB\rho_{B} lack entanglement only at one point (q=1/2q=1/2) of the corresponding domain, compare with Figures 3(a) and 3(d).

Figure 8(b) shows the result of applying LL and ε\varepsilon to the convex combinations ρB\rho_{B} of Bell–states exhibited in Figures 3(a) and 3(d). This time the optimization is over almost the entire domain of qq, mainly in the neighborhoods of q=0q=0 and q=1q=1, which serve as accumulation points. These systems are separable only for q=1/2q=1/2.

On the other hand, applying LL and ε\varepsilon to the generalized Werner–states shown in Figure 3 produces results that depend on ss, as expected. In Figure 9 we see that the maximum of LL and ε\varepsilon decreases with s<1s<1. Furthermore, the interval of qq for which LL is equal to zero becomes increasingly larger. Thus, any perturbation that modifies the original statistical mixture (i.e., the value s=1s=1) drastically affects entanglement: as mixing is maximized, the system loses quantum properties, making it increasingly classical.

Refer to caption
(a) s=3/4s=3/4
Refer to caption
(b) s=1/2s=1/2
Figure 9: The geometric measure LL (dotted curve) and entanglement of formation ε\varepsilon (continuous curve) applied to the generalized Werner–states shown in Figure 3. The case depicted in Figure 8(b) is recovered if s=1s=1. In general, the maximum values of LL and ε\varepsilon decrease with ss while the region where they become zero increases.

Another way to investigate the transition from entangled to separable configurations of a given state ρ\rho is to use the concept of robustness [8], which quantifies entanglement with respect to the maximally mixed state ρ\rho_{\star} and may be expressed in terms of the concurrence [14]. Referring to the optimized states of two qubits derived in the previous sections, the main point is to consider the density operator

ρ~X=(1ω)ρX+ωρ,w[0,1].\widetilde{\rho}_{X}=(1-\omega)\rho_{X}+\omega\rho_{\star},\quad w\in[0,1]. (42)

The robustness of the optimized ρX\rho_{X} corresponds to the minimal value of ω\omega, written ω0\omega_{0}, for which ρ~X\widetilde{\rho}_{X} becomes disentangled [8, 14]. The most important feature of ρ~X\widetilde{\rho}_{X} is that it is also X–shaped. Therefore, the LL–measure (34) is automatically applicable. A simple calculation yields

L(ρ~B)=2max{0,(1ω)L1(ρB)ω4,(1ω)L2(ρB)ω4},\displaystyle L(\widetilde{\rho}_{B})=2\max\left\{0,(1-\omega)L_{1}(\rho_{B})-\frac{\omega}{4},(1-\omega)L_{2}(\rho_{B})-\frac{\omega}{4}\right\}, (43)
L(ρ~Wk)=2max{0,(1ω)L1(ρWk)ω4},\displaystyle L(\widetilde{\rho}_{W_{k}})=2\max\left\{0,(1-\omega)L_{1}(\rho_{W_{k}})-\frac{\omega}{4}\right\}, (44)
L(ρ~S)=2max{0,(1ω)L1(ρS)ω4,(1ω)L2(ρS)ω4},\displaystyle L(\widetilde{\rho}_{S})=2\max\left\{0,(1-\omega)L_{1}(\rho_{S})-\frac{\omega}{4},(1-\omega)L_{2}(\rho_{S})-\frac{\omega}{4}\right\}, (45)

where Lj(ρX)L_{j}(\rho_{X}) stands for the first (j=1j=1) and second (j=2j=2) subtractions occurring in the LL-measures (35)-(37). Assuming that subtraction Lj(ρX)>0L_{j}(\rho_{X})>0 defines the value of L(ρX)L(\rho_{X}), we obtain the robustness of the optimized states of two qubits:

ω0=Lj(ρX)Lj(ρX)+1/4.\omega_{0}=\frac{L_{j}(\rho_{X})}{L_{j}(\rho_{X})+1/4}. (46)

For the Werner–states shown in Figure 8(a), this expression takes the maximal value 4/5 at q=1q=1, and minimal value 0 if q1/3q\leq 1/3. These values correspond to the maximally entangled expression of ρWk\rho_{W_{k}} and a completely disentangled form of ρWk\rho_{W_{k}}, respectively. Similar conclusions are obtained for the two-Bell mixed states shown in Figure 8(b). In turn, the robustness of the generalized Werner–states shown in Figures 9(a) and 9(b) take the maximal values 3/4 and 2/3, respectively.

3.4 Time-dependent systems

To further extend the applicability of our treatment, we now study what happens to entanglement when the system is explicitly time-dependent.

Suppose we have at hand a pair of two-level atoms which are entangled in energy, say |ψ2at=|β3|\psi_{\operatorname{2at}}\rangle=|\beta_{3}\rangle. Let us place these atoms in independent, isolated and identical electromagnetic cavities, each of which containing exactly nn photons. The state of the entire system can be written as |Φ=12(|+,n|,n+|,n|+,n)|\Phi\rangle=\tfrac{1}{\sqrt{2}}\left(|+,n\rangle\otimes|-,n\rangle+|-,n\rangle\otimes|+,n\rangle\right), where |n|n\rangle represents the state of the quantized field contained in each cavity. Besides |+|0|+\rangle\equiv|0\rangle and ||1|-\rangle\equiv|1\rangle. Following [41, 42, 43], with γ\gamma a coupling factor, the time-evolved state acquires the form

|Φ(t)=cos(γtn+1)[cos(γtn)|φ1isin(γtn)|φ2]isin(γtn+1)[cos(γtn)|φ3isin(γtn)|φ4],\begin{array}[]{rl}|\Phi(t)\rangle&=\cos(\gamma t\sqrt{n+1}\/)\left[\cos(\gamma t\sqrt{n}\/)|\varphi_{1}\rangle-i\sin(\gamma t\sqrt{n}\/)|\varphi_{2}\rangle\right]\\[5.16666pt] &\quad-i\sin(\gamma t\sqrt{n+1}\/)\left[\cos(\gamma t\sqrt{n}\/)|\varphi_{3}\rangle-i\sin(\gamma t\sqrt{n}\/)|\varphi_{4}\rangle\right],\end{array}

with |φ1=|Φt=0|\varphi_{1}\rangle=|\Phi\rangle_{t=0}, and

|φ2=12(|+,n|+,n1+|+,n1|+,n),|φ3=12(|,n+1|,n+|,n|,n+1),|φ4=12(|,n+1|+,n1+|+,n1|,n+1).\begin{array}[]{l}|\varphi_{2}\rangle=\tfrac{1}{\sqrt{2}}\left(|+,n\rangle\otimes|+,n-1\rangle+|+,n-1\rangle\otimes|+,n\rangle\right),\\[5.16666pt] |\varphi_{3}\rangle=\tfrac{1}{\sqrt{2}}\left(|-,n+1\rangle\otimes|-,n\rangle+|-,n\rangle\otimes|-,n+1\rangle\right),\\[5.16666pt] |\varphi_{4}\rangle=\tfrac{1}{\sqrt{2}}\left(|-,n+1\rangle\otimes|+,n-1\rangle+|+,n-1\rangle\otimes|-,n+1\rangle\right).\end{array}

The reduced time-dependent diatomic state results

ρ2at(t)=Trfieldsρ(t)=(r11(t)0000y0(t)y(t)00y(t)y0(t)0000r44(t)),\rho_{\operatorname{2at}}(t)=\operatorname{Tr}_{\operatorname{fields}}\rho(t)=\left(\begin{array}[]{cccc}r_{11}(t)&0&0&0\\[1.72221pt] 0&y_{0}(t)&y(t)&0\\[1.72221pt] 0&y(t)&y_{0}(t)&0\\[1.72221pt] 0&0&0&r_{44}(t)\end{array}\right), (47)

where

y0(t)=12cos2(γtn+1)cos2(γtn)+12sin2(γtn+1)sin2(γtn)y_{0}(t)=\tfrac{1}{2}\cos^{2}\left(\gamma t\sqrt{n+1}\right)\cos^{2}\left(\gamma t\sqrt{n}\right)+\tfrac{1}{2}\sin^{2}\left(\gamma t\sqrt{n+1}\right)\sin^{2}\left(\gamma t\sqrt{n}\right)

and

y(t)=12cos2(γtn+1)cos2(γtn).y(t)=\tfrac{1}{2}\cos^{2}\left(\gamma t\sqrt{n+1}\right)\cos^{2}\left(\gamma t\sqrt{n}\right).

In turn, the extreme point x0=r11r44x_{0}=\sqrt{r_{11}r_{44}} is obtained from the matrix-elements

r11(t)=cos2(γtn+1)sin2(γtn),r44(t)=sin2(γtn+1)cos2(γtn).r_{11}(t)=\cos^{2}\left(\gamma t\sqrt{n+1}\right)\sin^{2}\left(\gamma t\sqrt{n}\right),\,\,r_{44}(t)=\sin^{2}\left(\gamma t\sqrt{n+1}\right)\cos^{2}\left(\gamma t\sqrt{n}\right).
Refer to caption
(a)
Refer to caption
(b)
Figure 10: (a) The geometric measure LL applied to the time-dependent diatomic state ρ2at\rho_{\operatorname{2at}} for γ=1\gamma=1 and n=10n=10. As time passes, LL decreases from 1 to zero and then increases until it is almost equal to 1. This process is repeated over and over again (b) Comparison of L(ρ2at)L(\rho_{\operatorname{2at}}) with the difference yx0y-x_{0}. Clearly, inequality y>x0y>x_{0} is violated in the same time intervals where L=0L=0.

The profile of the diatomic state ρ2at\rho_{\operatorname{2at}} fits the structure of ρy\rho_{\mathcal{M}_{y}} at any time. The LL-measure returns the value 1 at t=0t=0, where the diatomic system is in the Bell–state |β3|\beta_{3}\rangle. As time passes, LL decreases to zero and then increases until it is almost equal to 1. This process is repeated over and over again, see Figure 10(a). The time intervals where entanglement is zero coincide with the violation of inequality x0<yx_{0}<y, see Figure 10(b).

We now focus our attention on the reduced states of ρ2at\rho_{\operatorname{2at}}, which have the same entropy S(ρ1)=S(ρ2)S(\rho_{1})=S(\rho_{2}). In Figure 11 we have depicted the result of applying LL and ε\varepsilon to ρ2at\rho_{\operatorname{2at}}, together with the entropy S(ρ1,2)S(\rho_{1,2}). We see that SS reaches its maximum value at different times. Some of such moments define also the local maxima of LL and ε\varepsilon, but others are in time intervals where there is no entanglement. As it is well known, the latter means that finding reduced states of maximum mixing does not provide information about the entanglement (if any) of the entire system if it is in a mixed state. However, the minima of SS play a different role in the system we are dealing with.

The envelope formed by the minima of S establishes an upper limit for the entanglement measure. To our knowledge, this surprising property of entropy shared by reduced states has not been reported in the literature on the matter.

The phenomenon described above is also present when we use any other Bell–state as initial condition instead of |β3|\beta_{3}\rangle. If we start from |β4|\beta_{4}\rangle the structure of ρ2at\rho_{\operatorname{2at}} is similar to the one we find in (47). But starting from |β1,2|\beta_{1,2}\rangle we arrive at a diatomic state of the form ρx\rho_{\mathcal{M}_{x}}. In any case, what we find is that the envelope formed by the minima of SS represents an upper bound on the entanglement strength as time progresses.

Refer to caption
(a)
Refer to caption
(b)
Figure 11: The envelope formed by the minima of the one-qubit entropy (blue curve) defines an upper bound for the entanglement measures of the time-dependent diatomic state ρ2at\rho_{\operatorname{2at}} (a) The geometric measure LL is red-shaded (b) The entanglement of formation ϵ\epsilon is purple-shaded.

4 Conclusions

We have established the necessary conditions to study entanglement in two-qubit systems by using the minimum of essential parameters.

The idea has been to construct density operators whose reduced one-qubit states share the same entropy, regardless of whether the state of the entire system is pure or mixed. The latter leads to the identification of ρX\rho_{X} states that have the capacity to host pairs of identical populations while reducing the number of coherences involved.

With the above results we have constructed a convex representation that facilitates the study of entanglement in two-qubit systems. The description is purely geometric and is based on two of the main characteristics of the X–states:

i) To obtain positive semidefinite operators ρX\rho_{X}, the coherence amplitudes x=|r14|x=|r_{14}| and y=|r23|y=|r_{23}| should be bounded from above by the corresponding populations, x0=r11r44x_{0}=\sqrt{r_{11}r_{44}} and y0=r22r33y_{0}=\sqrt{r_{22}r_{33}}. Otherwise, ρX\rho_{X} is not a quantum state.

ii) To find entanglement, xx and yy should be bounded from below by the complementary populations, y0y_{0} and x0x_{0}, respectively. Otherwise, state ρX\rho_{X} is separable.

Taking full advantage of such representation we have introduced a geometric measure LL, which is defined as the distance between pp (the point under study) and the closest point qq that defines separable states. The more remote, the greater the entanglement.

The LL-measure reproduces the results of the Hill–Wootters generalized concurrence CC for states ρX\rho_{X}. That is, our results give CC a geometric meaning that is not obvious without the convex structure introduced in this work. What is even better is that, unlike CC, the geometric measure LL distinguishes the rank of states with maximum entanglement.

We have found that rank-3 states ρX\rho_{X} exhibit the strongest entanglement when x0x_{0} and y0y_{0} are nonzero and different from each other. These states have no locally producible quantum correlations since no rank-3 or rank-4 state can be produced by local operations of one of the parties on a classically correlated state [47, 49]. If x0=0x_{0}=0 and y=y0y=y_{0}, or y0=0y_{0}=0 and x=x0x=x_{0}, states ρX\rho_{X} are pure (rank-1) and yield strong entanglement. The Bell–states fall into this category by maximizing to 1 the result given by the measure LL. It seems that states of higher ranks are more useful for quantum information procedures [49]. In particular, states of rank-3 can be used to reconstruct pure states by a remote party [48]. In turn, rank-4 states (which inhabit the different entanglement regions of 𝒮\mathcal{S}) are useful for reconstructing arbitrary states [49].

Note that the universality of two-qubit X–states ensures the utility of our geometric representation for studying entanglement in any configuration of two-qubit states. Indeed, it has been shown that ‘for every two-qubit state there is a two-qubit X–state of same spectrum and entanglement, as measured by concurrence, negativity or relative entropy of entanglement’ [38]. In this sense, no entanglement is lost by avoiding certain coherences of the initial state ρ\rho during the optimization process that we have developed throughout this work. Therefore, a point of the convex set (27), rewritten here as

𝒮={(x,y)2;0|r14|+|r23|12},\mathcal{S}=\left\{(x,y)\in\mathbb{R}^{2};0\leq|r_{14}|+|r_{23}|\leq\tfrac{1}{2}\right\},

determines the matrix elements of a density operator ρX\rho_{X} that shares with a two-qubit state (or a family of two-qubit states) ρ\rho both the spectrum and the entanglement. Geometrically, 𝒮\mathcal{S} is nothing more than the right-triangle shown in Figure 1. Within the geometric formulation presented in this work, the populations of ρX\rho_{X} are assumed to be given. Therefore, the coherences r14r_{14}, r23r_{23} and their complex conjugates determine not only the eligibility of ρX\rho_{X} and ρ\rho as quantum states but also the possibility of finding entanglement.

The applicability of our method goes far beyond the time-independent systems typically discussed in the literature. We have also studied what happens to entanglement when the system depends explicitly on time. Within the geometric representation, the time-evolution of ρX\rho_{X} describes paths that transit between areas with different entanglement strength, even invading regions where the state becomes separable to return to the entanglement zones, and so on. The latter opens the possibility of manipulating and controlling entanglement in two-qubit systems by solving the quantum inverse problem [54], where one seeks to manipulate systems in order to force them to behave in a particular way. Recent results concerning global and genuine entanglement in three-qubit systems can be found in [18], for other applications see [55, 56, 57, 58, 59, 60, 61].

We have found another outstanding result for the time-dependent system studied here. The envelope formed by the minima of SS, the entropy of the reduced states, establishes an upper bound for the entanglement measures. To our knowledge, this surprising property has not been reported in the literature on the matter.

Appendix A

Proposition Q (proof). Let us write the density operator in the form ρ=k,j=14rkjΓkj\rho=\sum_{k,j=1}^{4}r_{kj}\,\Gamma^{kj}, where the dyadic operators Γkj=|ekej|\Gamma^{kj}=|e_{k}\rangle\langle e_{j}|, k,j{1,2,3,4}k,j\in\{1,2,3,4\}, correspond to 4-square matrices for which all the entries are zero except the one in the kkth row and the jjth column, which acquires the value 1 [62]. These operators obey the multiplication rule ΓijΓkm=δjkΓim\Gamma^{ij}\Gamma^{km}=\delta_{jk}\Gamma^{im}, and have the properties k=14Γkk=𝕀\sum_{k=1}^{4}\Gamma^{kk}=\mathbb{I}, (Γkj)=Γjk(\Gamma^{kj})^{\dagger}=\Gamma^{jk}, where 𝕀\mathbb{I} is the identity operator in \mathcal{H}. It is a matter of substitution to verify the expressions ρ2=k,j=14skmΓkm\rho^{2}=\sum_{k,j=1}^{4}s_{km}\Gamma^{km} and skm==14rkrms_{km}=\sum_{\ell=1}^{4}r_{k\ell}r_{\ell m}. Then, using the factorization rkj=αkαjr_{kj}=\alpha_{k}\alpha^{*}_{j}, together with the normalization of |ψ|\psi\rangle, we obtain ρ2=ρ\rho^{2}=\rho. Therefore Trρ2=1\operatorname{Tr}\rho^{2}=1. \blacksquare

\bullet The eigenvalues and eigenvectors of ρX\rho_{X} discussed in Section 2.1 are given by the expressions

Λ1=12[r11+r44+(r11+r44)24(x02x2)],Λ2=12[r11+r44(r11+r44)24(x02x2)],Λ3=12[r22+r33+(r22+r33)24(y02y2)],Λ4=12[r22+r33(r22+r33)24(y02y2)],\begin{array}[]{c}\Lambda_{1}=\frac{1}{2}\left[r_{11}+r_{44}+\sqrt{(r_{11}+r_{44})^{2}-4\left(x_{0}^{2}-x^{2}\right)}\right],\\[6.88889pt] \Lambda_{2}=\frac{1}{2}\left[r_{11}+r_{44}-\sqrt{(r_{11}+r_{44})^{2}-4\left(x_{0}^{2}-x^{2}\right)}\right],\\[6.88889pt] \Lambda_{3}=\frac{1}{2}\left[r_{22}+r_{33}+\sqrt{(r_{22}+r_{33})^{2}-4\left(y_{0}^{2}-y^{2}\right)}\right],\\[6.88889pt] \Lambda_{4}=\frac{1}{2}\left[r_{22}+r_{33}-\sqrt{(r_{22}+r_{33})^{2}-4\left(y_{0}^{2}-y^{2}\right)}\right],\end{array} (A-1)

and

|ϵ1=xeiθ|e1+(Λ1r11)|e4(Λ1r11)2+x2,|ϵ2=xeiθ|e1+(Λ2r11)|e4(Λ2r11)2+x2,|ϵ3=yeiϕ|e2+(Λ3r22)|e3(Λ3r22)2+y2,|ϵ4=yeiϕ|e2+(Λ4r22)|e3(Λ4r22)2+y2.\begin{array}[]{c}|\epsilon_{1}\rangle=\displaystyle\frac{xe^{i\theta}|e_{1}\rangle+(\Lambda_{1}-r_{11})|e_{4}\rangle}{\sqrt{(\Lambda_{1}-r_{11})^{2}+x^{2}}},\quad|\epsilon_{2}\rangle=\frac{xe^{i\theta}|e_{1}\rangle+(\Lambda_{2}-r_{11})|e_{4}\rangle}{\sqrt{(\Lambda_{2}-r_{11})^{2}+x^{2}}},\\[12.05554pt] |\epsilon_{3}\rangle=\displaystyle\frac{ye^{i\phi}|e_{2}\rangle+(\Lambda_{3}-r_{22})|e_{3}\rangle}{\sqrt{(\Lambda_{3}-r_{22})^{2}+y^{2}}},\quad|\epsilon_{4}\rangle=\frac{ye^{i\phi}|e_{2}\rangle+(\Lambda_{4}-r_{22})|e_{3}\rangle}{\sqrt{(\Lambda_{4}-r_{22})^{2}+y^{2}}}.\end{array} (A-2)

In the above expressions we have used the notation introduced in Section 2.1 for the convex set 𝒮\mathcal{S}. Namely, x0=r11r44x_{0}=\sqrt{r_{11}r_{44}}, r14=xeiθr_{14}=xe^{i\theta}, and y0=r22r33y_{0}=\sqrt{r_{22}r_{33}}, r23=yeiϕr_{23}=ye^{i\phi}.

\bullet Let us review the situation when the matrix-elements of ρX\rho_{X} fulfill Proposition Q. That is, when the X–state is pure. To satisfy (3), given that r13r_{13} and r34r_{34} have α3\alpha_{3} as a common factor, it will be enough to take α3=0\alpha_{3}=0 so that these two matrix-elements are equal to zero. Similarly, we take α2=0\alpha_{2}=0 to cancel r24r_{24} and r12r_{12}. These α\alpha-parameters also give r22=r33=0r_{22}=r_{33}=0, so the second identity of Eq. (4) is automatically satisfied. Furthermore, we immediately obtain r23=0r_{23}=0. Then, the X–state (5) is reduced to the projector ρX=|ψ14ψ14|\rho_{X}=|\psi_{14}\rangle\langle\psi_{14}|, with

|ψ14=α1|e1+α4|e4,|α1|2+|α4|2=1.|\psi_{14}\rangle=\alpha_{1}|e_{1}\rangle+\alpha_{4}|e_{4}\rangle,\quad|\alpha_{1}|^{2}+|\alpha_{4}|^{2}=1. (A-3)

If we also demand that the first identity of Eq. (4) holds, then |α1|=|α4||\alpha_{1}|=|\alpha_{4}| and λR=(12,12)\vec{\lambda}_{R}=(\frac{1}{2},\frac{1}{2}). After adjusting the phases and requiring orthogonality, from (A-3) we recover the first pair of Bell–states (7). Proceeding in a similar way, now eliminating α1\alpha_{1} and α4\alpha_{4}, we obtain another projector ρX=|ψ23ψ23|\rho_{X}=|\psi_{23}\rangle\langle\psi_{23}|, where

|ψ23=α2|e2+α3|e3,|α2|2+|α3|2=1.|\psi_{23}\rangle=\alpha_{2}|e_{2}\rangle+\alpha_{3}|e_{3}\rangle,\quad|\alpha_{2}|^{2}+|\alpha_{3}|^{2}=1. (A-4)

In this case, the second identity of Eq. (4) gives λL=(12,12)\vec{\lambda}_{L}=(\frac{1}{2},\frac{1}{2}), so that (A-4) leads to the second pair of Bell–states (8).

\bullet The convex optimization discussed in Section 3 requires Lagrange multipliers. Consider the function f(r11,r22,r33,r44)=r11r44+r22r33f(r_{11},r_{22},r_{33},r_{44})=\sqrt{r_{11}r_{44}}+\sqrt{r_{22}r_{33}}, together with the constraint

g(r11,r22,r33,r44)=r11+r22+r33+r441=0.g(r_{11},r_{22},r_{33},r_{44})=r_{11}+r_{22}+r_{33}+r_{44}-1=0. (A-5)

Using mm as the Lagrange multiplier associated with constraint gg, we have the system

fr11mgr11=r442r11r44m=0,fr22mgr22=r332r22r33m=0,fr33mgr33=r222r22r33m=0,fr44mgr44=r112r11r44m=0.\begin{array}[]{c}\frac{\partial f}{\partial r_{11}}-m\frac{\partial g}{\partial r_{11}}=\frac{r_{44}}{2\sqrt{r_{11}r_{44}}}-m=0,\quad\frac{\partial f}{\partial r_{22}}-m\frac{\partial g}{\partial r_{22}}=\frac{r_{33}}{2\sqrt{r_{22}r_{33}}}-m=0,\\[6.88889pt] \frac{\partial f}{\partial r_{33}}-m\frac{\partial g}{\partial r_{33}}=\frac{r_{22}}{2\sqrt{r_{22}r_{33}}}-m=0,\quad\frac{\partial f}{\partial r_{44}}-m\frac{\partial g}{\partial r_{44}}=\frac{r_{11}}{2\sqrt{r_{11}r_{44}}}-m=0.\end{array}

Therefore

m=r112r11r44=r222r22r33=r332r22r33=r442r11r44.m=\frac{r_{11}}{2\sqrt{r_{11}r_{44}}}=\frac{r_{22}}{2\sqrt{r_{22}r_{33}}}=\frac{r_{33}}{2\sqrt{r_{22}r_{33}}}=\frac{r_{44}}{2\sqrt{r_{11}r_{44}}}.

The simplest way to satisfy these equalities is by making r11=r44r_{11}=r_{44} and r22=r33r_{22}=r_{33}. In this case f=r11+r22f=r_{11}+r_{22}. Then, from (A-5) it is found that 1/21/2 is the maximum value we are looking for.

\bullet The rank of states ρx\rho_{\mathcal{M}_{x}} that are represented by matrices (30) is as follows

rank(ρx)|y0=0={3,r22=0orr33=02,r22=0andx=x02,r33=0andx=x02,r22=r33=01,r22=r33=0andx=x0\left.\operatorname{rank}(\rho_{\mathcal{M}_{x}})\right|_{y_{0}=0}=\left\{\begin{array}[]{rl}3,&r_{22}=0\,\operatorname{or}\,r_{33}=0\\ 2,&r_{22}=0\,\operatorname{and}\,x=x_{0}\\ 2,&r_{33}=0\,\operatorname{and}\,x=x_{0}\\ 2,&r_{22}=r_{33}=0\\ 1,&r_{22}=r_{33}=0\,\operatorname{and}\,x=x_{0}\\ \end{array}\right. (A-6)

In turn, the rank of states ρy\rho_{\mathcal{M}_{y}} that are represented by matrices (31) reads

rank(ρy)|x0=0={3,r11=0orr44=02,r11=0andy=y02,r44=0andy=y02,r11=r44=01,r11=r44=0andy=y0\left.\operatorname{rank}(\rho_{\mathcal{M}_{y}})\right|_{x_{0}=0}=\left\{\begin{array}[]{rl}3,&r_{11}=0\,\operatorname{or}\,r_{44}=0\\ 2,&r_{11}=0\,\operatorname{and}\,y=y_{0}\\ 2,&r_{44}=0\,\operatorname{and}\,y=y_{0}\\ 2,&r_{11}=r_{44}=0\\ 1,&r_{11}=r_{44}=0\,\operatorname{and}\,y=y_{0}\\ \end{array}\right. (A-7)

Author Contributions

Conceptualization O.R.-O.; methodology, formal analysis, investigation, original draft preparation and review, S.L.-H., C.Q. and O.R.-O.; editing, project administration and funding acquisition, O.R.-O. All authors have read and agreed to the published version of the manuscript.

Funding

This research was funded by Consejo Nacional de Humanidades, Ciencia y Tecnología (CONACHyT, Mexico), grant number A1-S-24569, and by Instituto Politécnico Nacional (IPN, Mexico), project SIP20242277.

Acknowledgment

S.L.-H acknowledges the support from CONAHCyT through the scholarship 592045.

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