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Basis-Dependent Quantum Nonlocality

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22 April 2024

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23 April 2024

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Abstract
Quantum nonlocality represents correlation properties between subsystems of a composite quantum system, usually including the four types: Bell nonlocality, steerability, entanglement, and quantum correlation (quantum discord). Given a basis $e_{AB}=\{|e_{ij}\>\}_{i\in[d_A],j\in[d_B]}$ for the Hilbert space $\H_A\otimes \H_B$ of a bipartite system $AB$, a density operator $\rho^{AB}$ (quantum state) of $AB$ can be represented as a $d_Ad_B\times d_Ad_B$ matrix $\hat{\rho}_{e_{AB}}=[\]$, called the density matrix of a density operator $\rho^{AB}$. A natural question is what is the relationship between the quantum nonlocality of a density operator $\rho^{AB}$ and its corresponding density matrix $\hat{\rho}_{e_{AB}}$? In this work, we discuss the relationships between quantum locality and basis, and prove that one type of quantum locality of density operators and that of their density matrices under a basis are the same if and only if the chosen basis is the tensor product of the bases of subsystems. Consequently, different bases define different quantum nonlocality density operators.
Keywords: 
Subject: Physical Sciences  -   Quantum Science and Technology

1. Introduction

Quantum nonlocality, also called quantum correlation, represents correlation properties between subsystems of a composite quantum system, including Bell nonlocality, steerability, entanglement, and quantum correlation.
Bell nonlocality of bipartite states is demonstrated by some local quantum measurements whose statistics of the measurement outcomes cannot be explained by a local hidden variable (LHV) model [1,2]. Such a nonclassical feature of quantum mechanics can be used in device-independent quantum information processing [2]. For more discussions on Bell nonlocality, please refer to Clauser and Shimony [3], Home and Selleri [4], Khalfin and Tsirelson [5], Tsirelson [6], Zeilinger [7], Werner and Wolf [8], Genovese [9], and Buhrman et al. [10], and [11,12,13,14].
Einstein-Podolsky-Rosen (EPR) steering, as a form of quantum correlation, was first observed by Schr o ¨ dinger [15] in the context of the well-known EPR paradox [16,17,18,19]. EPR steering arises in scenarios wherein some local quantum measurements on one part of a bipartite system are used to steer the other part. This scenario demonstrates EPR steering if the obtained ensembles cannot be explained by a local hidden state (LHS) model [20]. Following a close analogy of criteria for other forms of quantum nonlocality, Cavalcanti et al. [21] developed a general theory of experimental EPR steering criteria and derived several criteria applicable to discrete and continuous-variable observables. Saunders et al. [22] contributed experimental EPR steering by using Bell local states. Bennet et al. [23] derived arbitrarily loss-tolerant tests, thereby enabling us to perform a detection loophole free demonstration of EPR steering with parties separated by a coiled 1-km-long optical fiber. Händchen et al. [24] presented an experimental realization of two entangled Gaussian modes of light that shows a steering effect in one direction but not in the other. The generated one-way steering provides new insight into quantum physics and may open a new field of applications in quantum information. EPR steering, as an intermediate form of quantum correlation between entanglement and Bell nonlocality, allows for entanglement certification when the measurements performed by one of the parties are not characterized (or are untrusted); it has many applications, such as quantum key distribution [25,26,27], quantum benchmark for qubit teleportation[28], subchannel discrimination in a quantum evolution [29], and so on. Therefore, it has been widely researched, see [30,31,32,33,34,35,36,37,38,39].
Just like quantum steering, quantum entanglement was also recognized by Einstein, Podolsky, Rosen [16], and Schr o ¨ dinger [15] in 1935. It is a property of a composite quantum system involving nonclassical correlations between subsystems and then having potential for many quantum processes, including canonical ones: quantum cryptography, quantum teleportation, and dense coding.
A bipartite entanglement state reveals correlations between the two subsystems. However, some separable states may reveal some correlations. Such states are just the states that have nonzero quantum discord. Quantum discord induced by H. Ollivier and W.H. Zurek in [40] is a measure of the quantumness of correlations but not a quantum property of states. Considered measurement-induced disturbance, Luo [41] classified correlations between subsystems into classical correlations and quantum correlations by introducing classical correlated (CC) states and quantum correlated states. It was found that a CC state is a separable state [40,41,42,43] and so any entangled state must be a QC state. Thus, quantum correlations have been applied in some quantum computing tasks without entanglement [44], the study of quantum key distribution [45], three-spin XXZ chain with three-spin interaction [46] and so on.
It is well-known that the four types of quantum nonlocality have the following relations:
Bell nonlocality steerability entanglement quantum correlation ,
equivalently,
Bell locality unsteerability separability classical correlation .
From the mathematical definitions of quantum locality (Bell locality, separability and classical correlation), we see that these properties depend only on the algebraic structures of the density operators ρ A B (quantum states) and should be independent of the choice of basis for the Hilbert space H A H B of a system A B . However, in applications and experiments, density operators are usually written as matrices under a chosen basis e A B for H A H B . As we known, different bases lead to different matrix representations of operators. Thus, different choice of bases may induce different quantum locality of density matrices, which we called basis-dependent quantum nonlocality.
In the sequence sections, we discuss the relationships between these quantum locality and basis, and find that quantum locality of density operators and their density matrices under a basis are the same only when the basis is a tensor product of the bases of subsystems.

2. Basis Dependent Separability

According to quantum mechanics, a quantum system S is described by a d S -dimensional complex Hilbert space H S (called the state space of S) with a right-linear inner product · | · and the states of the system are denoted by positive operators of trace 1 on H S . The set of all states of S is denoted by D ( H S ) . Thus,
D ( H S ) = { ρ B ( H S ) : ρ 0 , tr ρ = 1 } ,
where B ( H S ) is the C * -algebra of all bounded linear operators on H S . The elements of D ( H S ) are called the mixed states of S. A unit vector | ψ in H S is said to be a pure state of S and the set of all pure states of S is denoted by P S ( H S ) . We also use [ d ] to denote the set { 1 , 2 , , d } .
By the postulates of quantum mechanics, the state space of the composite system A B of A and B is given by the tensor product space H A H B of the state spaces H A and H B of A and B, respectively.

2.1. Concepts and Notations

Recall that a state ρ D ( H A H B ) is said to be separable if it can be written as the form of
ρ = i = 1 k c i ρ i A ρ i B
for some states ρ i A D ( H A ) , ρ i B D ( H B ) and c i 0 ( i [ k ] ) with i = 1 k c i = 1 . Otherwise, it is said to be entangled. Moreover, a pure state | ψ P S ( H A H B ) is said to be separable if it can be written as the form | ψ = | ψ A | ψ B for some | ψ A P S ( H A ) and | ψ B P S ( H B ) . Otherwise, it is called to be entangled.

2.2. Separability Depending on Basis

Let e A B = { | e i j : i [ d A ] , j [ d B ] } be an orthonormal basis (ONB) for H A H B and U : H A H B C d A d B = C d A C d B be the coordinate mapping:
U | ψ A B = ( c 11 , c 12 , , c 1 d B , c 21 , c 22 , , c 2 d B , , c d A 1 , c d A 2 , , c d A d B ) T
for all | ψ A B = i , j c i j | e i j in H A H B . We call the vector U | ψ A B the coordinate state of a state | ψ A B of H A H B .
We want to discuss the relationship between the separability of the coordinate state U | ψ A B and that of the original (abstract) state | ψ A B . For convenience, we write U | ψ A B = | ψ A B e A B . Let { | i A } i = 1 d A and { | j B } j = 1 d B be the canonical { 0 , 1 } -bases for C d A and C d B , respectively. Then we get the canonical { 0 , 1 } -basis (with m = d A , n = d B )
{ | i A j B } i , j = { | 1 A 1 B , | 1 A 2 B , , | 1 A n B , , | m A 1 B , | m A 2 B , , | m A n B }
for C d A C d B . Thus, the definition (2) of U becomes
U | ψ A B = i , j c i j | i A j B
for all | ψ A B = i , j c i j | e i j in H A H B . For example,
U | e i j = | i A | j B | i A | j B | i A j B , i [ d A ] , j [ d B ] ,
leading to
i A j B | U ρ A B U | k A B = e i j | ρ A B | e k = i A j B | ρ e A B A B | k A B
for all i , k [ d A ] , j , [ d B ] , where ρ e A B A B : = [ e i j | ρ A B | e k ] is the d A d B × d A d B matrix with ( i j , k ) -entry e i j | ρ A B | e k , called the density matrix of ρ A B under basis e A B and written as ρ e A B A B = U ρ A B U due to the relation (5).
Equation (4) shows that the coordinate mapping U transforms the basis states | e i j as separable states | i A | j B . Generally, U | ψ A B is not necessarily separable even if | ψ A B is separable. For example, we let d A = d B = 2 and e A = { | e i A } i = 1 2 and e B = { | e i B } i = 1 2 for H A and H B , respectively, and define an ONB e A B = { | e 11 , | e 12 , | e 21 , | e 22 } for H A H B by
| e 11 = 2 2 ( | e 1 A e 1 B + | e 2 A e 2 B ) ; | e 12 = 2 2 ( | e 1 A e 2 B + | e 2 A e 1 B ) ; | e 21 = 2 2 ( | e 1 A e 2 B | e 2 A e 1 B ) ; | e 22 = 2 2 ( | e 1 A e 1 B | e 2 A e 2 B ) .
Clearly, | ψ A B : = | e 1 A e 1 B = 2 2 ( | e 11 + | e 22 ) is a separable state of H A H B , but
U | ψ A B = | ψ A B e A B = 2 2 , 0 , 0 , 2 2 T C 2 C 2 ,
which can not be written as a tensor product of two qubits and then not separable. If, however, we choose a “separable basis":
e A e B = { | e i A | e j B } i , j = 1 2 = { | e 1 A | e 1 B , | e 1 A | e 2 B , | e 2 A | e 1 B , | e 2 A | e 2 B } ,
then the coordinate state of | ψ A B = | e 1 A e 1 B = 2 2 ( | e 11 + | e 22 ) reads
| ψ A B e A e B = 1 , 0 , 0 , 0 T C 2 C 2 ,
which is separable.
This observation leads to the following conclusion.
Theorem 1. 
Let e A B = { | e i j : i [ d A ] , j [ d B ] } where | e i j = | e i A | e j B ( i [ d A ] , j [ d B ] ) for some ONBs e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively. Then
(a) A pure state | ψ A B is a separable state of H A H B if and only if its coordinate state | ψ A B e A B is a separable state of C d A C d B .
(b) A density operator ρ A B is a separable state of H A H B if and only if its density matrix ρ e A B A B is a separable state of C d A C d B .
Proof. ( a ) For every separable state | ψ A B = | ψ A | ψ B , it holds that
c i j : = e i j | ψ A B = e i A | ψ A · e j B | ψ B
for all i , j . Writing a i = e i A | ψ A and b j = e j B | ψ B implies that
| ψ A B e A B = ( a 1 , a 2 , , a d A ) T ( b 1 , b 2 , , b d B ) T ,
and so | ψ A B e A B is a separable state in C d A C d B .
Conversely, let | ψ A B e A B be a separable state. Then Equation (6) holds for some states | a = ( a 1 , a 2 , , a d A ) T and | b = ( b 1 , b 2 , , b d B ) T of C d A and C d B , respectively. Put | ψ A = i = 1 d A a i | e i A and | ψ B = j = 1 d B b j | e j B , then U ( | ψ A | ψ B ) = | a | b = U | ψ A B and so | ψ A B = | ψ A | ψ B since U is injective. Hence, | ψ A B is separable. This shows that U | ψ A B = | ψ A B e A B is separable if and only if ψ A B is separable.
( b ) First, we let ρ A B = t c t ρ t A ρ t B be a separable state of A B . Then
[ e i j | ρ A B | e k ] = t c t [ e i A | ρ t A | e k A · e j B | ρ t B | e B ] = t c t [ e i A | ρ t A | e k A ] [ e j B | ρ t B | e B ] ,
which is the tensor product of two density matrices. Thus, ρ e A B A B is a separable density matrix. □
Conversely, we let ρ e A B A B be a separable density matrix. Then ρ e A B A B = n = 1 m t n [ a i k ( n ) ] [ b j ( n ) ] for some density matrices [ a i k ( n ) ] and [ b j ( n ) ] where t n 0 and n t n = 1 . Define density operators ρ n A on H A and ρ n B on H B by
e i A | ρ n A | e k A = a i k ( n ) , e j B | ρ n B | e B = b j ( n ) ,
for all i , j , k , , then we compute that
e i j | n = 1 m t n ( ρ n A ρ n B ) | e k = n = 1 m t n [ e i A | ρ n A | e k A · e j B | ρ n B | e B ] = n = 1 m t n [ e i A | ρ n A | e k A ] [ e j B | ρ n B | e B ] = n = 1 m t n [ a i k ( n ) ] i , k [ b j ( n ) ] = ρ e A B A B = [ e i j | ρ A B | e k ] ,
and so ρ A B = n = 1 m t n ( ρ n A ρ n B ) , which is separable. The proof is completed.
Similarly, one can check the following.
Theorem 2. 
Let d A = d B = d , e A B = { | e i j : i [ d A ] , j [ d B ] } where | e i j = | e j A | e i B ( i [ d A ] , j [ d B ] ) for some ONBs e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively. Then
(a) A pure state | ψ A B is separable if and only if its coordinate state | ψ A B e A B is separable.
(b) A density operator ρ A B is separable if and only if its density matrix ρ e A B A B is separable.
The following theorem shows that the condition | e i j = | e i A | e j B (resp. | e i j = | e j A | e i B ) is necessary for the conditions ( a ) and ( b ) in Theorem 1 (resp. Theorem 2) to be satisfied.
Theorem 3. 
Let e A B = { | e i j : i [ d A ] , j [ d B ] } be an orthonormal basis for H A H B and and U be fined by Equation (2). Then the following statements are equivalent (TFSAE).
(a) The coordinate mapping U preserves separability of pure states in both directions, i.e., | ψ A B is separable if and only if U | ψ A B is separable.
(b) The coordinate mapping U preserves separability of density operators in both directions, i.e., a density operator ρ A B is separable if and only if its density matrix ρ e A B A B is separable.
(c) There exist unitary operators W X : H X C d X ( X = A , B ) such that when d A d B , U = W A W B ; when d A = d B = d , either U = W A W B , or U = S ( W A W B ) , where S : C d C d is the swap operator: S ( | x | y ) = | y | x .
(d) There exist orthonormal bases e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively, such that when d A d B , | e i j = | e i A | e j B for all i , j ; When d A = d B = d , either | e i j = | e i A | e j B for all i , j , or | e i j = | e j A | e i B for all i , j .
Proof. ( a ) ( b ) : Suppose that ( a ) holds. Let ρ A B = n = 1 m c n ρ n A ρ n B be a convex combination of product states. It suffices to prove that U ( ρ n A ρ n B ) U is separable for each n. Fixed n and write
ρ n A = s λ s | ψ s A ψ s A | , ρ n B = t μ t | ψ t B ψ t B | ,
then
U ( ρ n A ρ n B ) U = s , t λ s μ t U | ψ s A ψ t B ψ s A ψ t B | U ,
which is separable using ( a ) . Hence, U ρ A B U = n = 1 m c n U ( ρ n A ρ n B ) U is separable. It follows from Theorem 1 ( b ) that the density matrix [ i A j B | U ρ A B U | k A B ] is separable, i.e., ρ e A B A B : = [ e i j | ρ A B | e k ] is separable. Conversely, let [ e i j | ρ A B | e k ] be separable. Then the density matrix [ i A j B | U ρ A B U | k A B ] is separable and therefore the density operator U ρ A B U is separable (Theorem 1 ( b ) ). Thus, we can write U ρ A B U = n c n | α n A B α n A B | for some separable pure states | α n A B of C d A C d B , where c n 0 with n c n = 1 . Since ρ A B = n c n U | α n A B α n A B | U and U | α n A B is separable (using ( a ) ) for all n, we see that ρ A B is separable. Now, ( b ) follows. Clearly, ( b ) implies ( a ) . □
( a ) ( c ) : Take ONBs e A = { | x i } i = 1 d A and e B = { | y j } j = 1 d B for H A and H B , respectively, and define unitary operators U A : H A C d A and U B : H B C d B by
U A i = 1 d A c i | x i = ( c 1 , c 2 , , c d A ) T ,
U B j = 1 d B d j | y j = ( d 1 , d 2 , , d d A ) T ,
and put U A B = U A U B , V = U U A B 1 . Then we obtain a commutative diagram Figure 1:
Let ( a ) be valid. Since both U and U A B preserve separability of pure states in both directions, so does V, i.e., V | ψ is separable if and only if | ψ is separable. It follows from [47] that there are unitary operators V A on C d A and V B on C d B such that when d A d B , V = V A V B ; when d A = d B = d , either V = V A V B , or V = S ( V A V B ) . Thus, condition ( c ) follows by letting W X = V X U X ( X = A , B ). See Figure 2 for the last case.
( c ) ( d ) : Suppose that condition ( c ) is satisfied. From the definition of U, we see that U | e i j = | i A | j B for all i [ d A ] and j [ d B ] where { | i A } i = 1 d A and { | j B } j = 1 d B are the canonical { 0 , 1 } -bases for C d A and C d B , respectively. Put | e i A = W A 1 | i A and | e j B = W B 1 | j B for all i , j .
When d A d B , we have
| e i A | e j B = W A 1 | i A W B 1 | j B = U 1 ( | i A | j B ) = | e i j
for all i , j ;
When d A = d B = d , if U = W A W B , then we have
| e i A | e j B = W A 1 | i A W B 1 | j B = U 1 ( | i A | j B ) = | e i j
for all i , j ; if U = S ( W A W B ) , then we have
| e j A | e i B = W A 1 | j A W B 1 | i B = U 1 S ( | j A | i B ) = U 1 ( | i B | j A ) = U 1 ( | i A | j B ) = | e i j
for all i , j , here the fact that | i B = | i A and | j A = | j B were used. Now, condition ( d ) follows.
( d ) ( a ) : Suppose that condition ( d ) is satisfied. Let | ψ A and | ψ B be any states of H A and H B , respectively. Then
| ψ A = i = 1 d A c i | e i A , | ψ B = j = 1 d B d j | e j B .
When | e i j = | e i A | e j B for all i , j , we have
U ( | ψ A | ψ B ) = i , j c i d j U ( | e i A | e j B ) = i , j c i d j U | e i j = i , j c i d j | i A | j B = | u | v ,
where | u = i c i | i A and | v = j d j | j B .
When | e i j = | e j A | e i B for all i , j , we have d A = d B = d and write
| ψ A = j = 1 d d j | e j A , | ψ B = i = 1 d c i | e i B .
Thus,
U ( | ψ A | ψ B ) = i , j c i d j U ( | e j A | e i B ) = i , j c i d j U | e j i = i , j c i d j | j A | i B = | u | v ,
where | u = i c i | i A and | v = j d j | j B . This shows that U maps any separable pure state as a separable pure state.
Conversely, we assume that U | ψ A B = | u | v for some states | u and | v of C d A and C d B , respectively. Let us show that | ψ A B is separable. To do this, we let
| ψ A B = i , j t i j | e i j , | u = i c i | i A , | v = j d j | j B .
Then
i , j c i d j | i A | j B = | u | v = U | ψ A B = i , j t i j | i A | j B
and so t i j = c i d j for all i , j . Hence, | ψ A B = i , j c i d j | e i j . Since either | e i j = | d i A | e j B for all i , j , or d A = d B = d and | e i j = | e j A | e i B for all i , j , we have either
| ψ A B = i = 1 d c i | e i A j = 1 d d j | e j B ,
or
| ψ A B = j = 1 d d j | e j A i = 1 d c i | e i B .
This shows that | ψ A B is separable. Thus, U preserves separability of pure states in both directions and so condition ( a ) is satisfied. The proof is completed.

3. Basis Dependent Bell Locality

In this section, we will discuss relationship between Bell locality and basis. To describe and discuss Bell locality, the following mathematical definitions were given by [14] abstracted from the literatures [2,20].

3.1. Concepts and Notations

To describe Bell locality of a bipartite state ρ A B , we use x and y to denote the labels of POVMs of Alice and Bob and use a and b to denote their measurement outcomes, respectively. Thus, their POVM choices are denoted by M x = { M a | x } a = 1 o A and N y = { N b | y } b = 1 o B , respectively, where x [ m A ] , y [ m B ] . These POVMs form measurement assemblages (MA) of A and B: M A = { M x } x = 1 m A and N B = { N y } y = 1 m B , respectively.
The following concepts were given in [14].
(1) A state ρ A B is said to be Bell local for a given measurement assemblage ( M A , N B ) if there exists a probability distribution (PD) { π λ } λ = 1 d such that, for each ( λ , x ) and ( λ , y ) , there exist PDs { P A ( a | x , λ ) } a = 1 o A and { P B ( b | y , λ ) } b = 1 o B , respectively, for which it holds that
tr [ ( M a | x N b | y ) ρ A B ] = λ = 1 d π λ P A ( a | x , λ ) P B ( b | y , λ )
for all a , b , x , y .
Equation (7) is said to be a local hidden variable model (LHVM) of ρ A B w.r.t. MA ( M A , N B ) and λ is said to be an LHV with PD { π λ } λ = 1 d .
(2) A state ρ A B is said to be Bell nonlocal for ( M A , N B ) if it is not Bell local for ( M A , N B ) .
(3) A state ρ A B is said to be Bell local if for every ( M A , N B ) , there exists a PD { π λ } λ = 1 d such that Equation (7) holds.
(4) A state ρ A B is said to be Bell nonlocal if it is not Bell local, i.e., ρ A B is not Bell local for some ( M A , N B ) .
Let BL ( M A , N B ) denote the set of all states that are Bell local for M A N B , BNL ( M A , N B ) denote the set of all states that are Bell nonlocal for ( M A , N B ) , BL ( A B ) the set of all Bell local states of A B ; BNL ( A B ) denote the set of all states that are Bell nonlocal. Thus, we see from the definition that
BL ( A B ) = M A , N B BL ( M A , N B ) ; BNL ( A B ) = M A , N B BNL ( M A , N B ) .

3.2. Bell Locality Depending on Basis

Let e A B = { | e i j : i [ d A ] , j [ d B ] } where | e i j = | e i A | e j B ( i [ d A ] , j [ d B ] ) for some ONBs e A = { | e i A } i = 1 d A and e B = { | e i A } i = 1 d A for H A and H B , respectively. Define unitary operators:
U A : H A C d A , U A i = 1 d A c i | e i A = ( c 1 , c 2 , , c d A ) T ,
U B : H B C d B , U B j = 1 d B d j | e j B = ( d 1 , d 2 , , d d A ) T ,
and for every linear operator T : H A H B H A H B , define a d A d B × d A d B matrix
T ˜ = [ t i j , k ] with ( i j , k ) entry t i j , k = e i A e j B | T | e k A e B .
Since
i A j B | ( U A U B ) T ( U A U B ) | k A B = e i A e j B | T | e k A e B = t i j , k = i A j B | T ˜ | k A B
for all i , j , k , we have
tr ( T ˜ ) = tr ( ( U A U B ) T ( U A U B ) ) .
Let M A = { M x } x = 1 m A and N B = { N y } y = 1 m B be measurement assemblages (MAs) of H A and H B , respectively, where M x = { M a | x } a = 1 o A and N y = { N b | y } b = 1 o B are POVMs of systems A and B, respectively. Then M x ˜ : = { M a | x ˜ } a = 1 o A and N y ˜ = { N b | y ˜ } b = 1 o B are POVMs of systems C d A and C d B , respectively, where
M a | x ˜ = U A M a | x U A , N b | y ˜ = U B N a | x U B .
Hence, M A ˜ = { M x ˜ } x = 1 m A and N B ˜ = { N y ˜ } y = 1 m B be MAs of C d A and C d B , respectively. Using Equation (10) yields that for all x , y , a , b ,
tr [ ( M a | x ˜ N b | y ˜ ) ρ e A B A B ] = tr [ ( M a | x N b | y ) ρ A B ] .
Thus, ρ A B BL ( M A , N B ) if and only if ρ e A B A B BL ( M A ˜ , N B ˜ ) . Since Bell locality and separability of pure states are the same [48] for pure states, we see from Theorem 1 ( a ) that a pure state | ψ A B in H A H B is Bell local if and only if its coordinate state | ψ A B e A B is Bell local.
As a conclusion, we obtain the following.
Theorem 4. 
Let e A B = { | e i j : i [ d A ] , j [ d B ] } where | e i j = | e i A | e j B ( i [ d A ] , j [ d B ] ) for some ONBs e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively. Then
(a) A pure state | ψ A B is a Bell local state of H A H B if and only if its coordinate state | ψ A B e A B is a Bell local state of C d A C d B .
(b) A density operator ρ A B is a Bell local state of H A H B if and only if its density matrix ρ e A B A B : = [ e i j | ρ A B | e k ] is a Bell local state of C d A C d B = C d A d B with ( i j , k ) -entry e i j | ρ A B | e k .
Similarly, one can check the following.
Theorem 5. 
Let d A = d B = d , e A B = { | e i j : i [ d A ] , j [ d B ] } where | e i j = | e j A | e i B ( i [ d A ] , j [ d B ] ) for some ONBs e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively. Then
(a) A pure state | ψ A B is a Bell local state of H A H B if and only if its coordinate state | ψ A B e A B is a Bell local state of C d A C d B .
(b) A density operator ρ A B is Bell local if and only if its density matrix ρ e A B A B : = [ e i j | ρ A B | e k ] is Bell local with ( i j , k ) -entry e i j | ρ A B | e k .
Using Theorem 3, Theorems 4 and 5, once can check the following.
Theorem 6. 
Let e A B = { | e i j : i [ d A ] , j [ d B ] } be an orthonormal basis for H A H B and and U be fined by Equation (2). Then TFSAE.
(a) The coordinate mapping U preserves Bell locality of pure states in both directions, i.e., | ψ A B is Bell local if and only if U | ψ A B is Bell local.
(b) A density operator ρ A B is Bell local if and only if its density matrix ρ e A B A B : = [ e i j | ρ A B | e k ] is Bell local with ( i j , k ) -entry e i j | ρ A B | e k .
(c) There exist unitary operators W X : H X C d X ( X = A , B ) such that when d A d B , U = W A W B ; when d A = d B = d , either U = W A W B , or U = S ( W A W B ) , where S : C d C d is the swap operator: S ( | x | y ) = | y | x .
(d) There exist orthonormal bases e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively, such that when d A d B , | e i j = | e i A | e j B for all i , j ; When d A = d B = d , either | e i j = | e i A | e j B for all i , j , or | e i j = | e j A | e i B for all i , j .
Proof. 
Use the implications:
( a ) ( d ) ( Theorem ) , ( d ) ( c ) ( Theorem ) , ( d ) ( b ) ( Theorems and ) , ( b ) ( a ) .

4. Basis Dependent Unsteerability

In this section, we will discuss relationship between unsteerability and basis.

4.1. Concepts and Notations

Recall that [14] a state ρ A B of H A H B is said to be unsteerable from A to B with an MA M A = { M x } x = 1 m A where M x = { M a | x } a = 1 o A is a POVM of system A if there exists a PD { π λ } λ = 1 n and a set { σ λ } λ = 1 n of system B such that
tr A [ ( M a | x I B ) ρ A B ] = λ = 1 n π λ P A ( a | x , λ ) σ λ , x , a ,
where { P A ( a | x , λ ) } a = 1 o A is a PD for all x , λ . ρ A B is said to be unsteerable from A to B if it is unsteerable from A to B with any MA M A . ρ A B is said to be steerable from A to B if it is not unsteerable for some MA M A . A pure state | ψ A B is said to be unsteerable from A to B if so is its density operator | ψ A B ψ A B | . Similarly, one define unsteerability from B to A. It is easy to see that a state that is unsteerable either from A to B or from B to A is Bell local. Thus, a pure state is unsteerable either from A to B or from B to A is separable.

4.2. Unsteerability Depending on Basis

Let e A B = { | e i j : i [ d A ] , j [ d B ] } where | e i j = | e i A | e j B ( i [ d A ] , j [ d B ] ) for some ONBs e A = { | e i A } i = 1 d A and e B = { | e i A } i = 1 d A for H A and H B , respectively. Then a density operator ρ A B on H A H B has the corresponding density matrix ρ e A B A B of ρ A B under the basis e A B = e A e B is
ρ e A B A B = ( U A U B ) ρ A B ( U A U B ) ,
where U A and U B are unitary operators given by Equations (8) and (9). In this case, for any MA M A of system A, we have
tr A [ ( M a | x ˜ E d B ) ρ e A B A B ] = tr A [ ( M a | x I B ) ρ A B ] ,
where E d B is the d B × d B unit matrix. Thus, ρ A B is unsteerable from A to B (resp. with MA M A = { M x } x = 1 m A ) if and only if its density matrix ρ e A B A B is unsteerable from A to B (resp. with MA M A ˜ : = { M x ˜ } x = 1 m A ).
Similarly, when d A = d B = d and | e i j = | e j A | e i B for all i , j [ d ] , we have
ρ e A B A B = S ( U A U B ) ρ A B ( U A U B ) S ,
where S is the swap operator on C d C d . Thus,
tr B [ ( E d A M a | x ˜ ) ρ e A B A B ] = tr A [ ( M a | x I B ) ρ A B ] .
This shows that ρ A B is unsteerable from A to B (resp. with MA M A = { M x } x = 1 m A ) if and only if its density matrix ρ e A B A B is unsteerable from B to A (resp. with MA M A ˜ : = { M x ˜ } x = 1 m A ).
From these observations, we obtain the following.
Theorem 7. 
Let e A B = { | e i j : i [ d A ] , j [ d B ] } where | e i j = | e i A | e j B ( i [ d A ] , j [ d B ] ) for some ONBs e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively. Then
(a) A pure state | ψ A B is unsteerable from A to B if and only if its coordinate state | ψ A B e A B is unsteerable from A to B.
(b) A density operator ρ A B is unsteerable from A to B if and only if its density matrix ρ e A B A B : = [ e i j | ρ A B | e k ] is unsteerable from A to B.
Theorem 8. 
Let d A = d B = d , e A B = { | e i j : i [ d A ] , j [ d B ] } where | e i j = | e j A | e i B ( i [ d A ] , j [ d B ] ) for some ONBs e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively. Then
(a) A pure state | ψ A B is unsteerable from A to B if and only if its coordinate state | ψ A B e A B is unsteerable from B to A.
(b) A density operator ρ A B is unsteerable from A to B if and only if its density matrix ρ e A B A B : = [ e i j | ρ A B | e k ] is unsteerable from B to A.
Using Theorem 1 and the fact that a pure state | ψ A B is unsteerable from A to B if and only if it is separable [48], combining Theorem 7, one can check the following.
Theorem 9. 
Let d A d B and e A B = { | e i j : i [ d A ] , j [ d B ] } be an orthonormal basis for H A H B and and U be defined by Equation (2). Then TFSAE.
(a) | ψ A B is unsteerable from A to B if and only if U | ψ A B is unsteerable from A to B.
(b) A density operator ρ A B is unsteerable from A to B if and only if its density matrix ρ e A B A B : = [ e i j | ρ A B | e k ] is unsteerable from A to B.
(c) There exist unitary operators W X : H X C d X ( X = A , B ) such that when d A d B , U = W A W B .
(d) There exist orthonormal bases e A = { | e i A } i = 1 d A and e B = { | e i A } i = 1 d A for H A and H B , respectively, such that | e i j = | e i A | e j B for all i , j .
Using Theorem 1 and the fact that a pure state | ψ A B is unsteerable from A to B if and only if it is separable [48], combining Theorem 8, one can check the following.
Theorem 10. 
Let d A = d B = d and e A B = { | e i j : i [ d A ] , j [ d B ] } be an orthonormal basis for H A H B and U be defined by Equation (2). Then the following (a) and (b) are equivalent.
(a) | ψ A B is unsteerable from A to B if and only if U | ψ A B is unsteerable from A to B.
(b) A density operator ρ A B is unsteerable from A to B if and only if its density matrix ρ e A B A B : = [ e i j | ρ A B | e k ] is unsteerable from A to B.
If (a) or (b) holds, then
(c) There exist unitary operators W X : H X C d X ( X = A , B ) such that U = W A W B , or U = S ( W A W B ) .
(d) There exist orthonormal bases e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively, such that | e i j = | e i A | e j B for all i , j , or | e i j = | e j A | e i B for all i , j .

5. Basis Dependent Classical Correlation

In this section, we will discuss relationship between classical correlation and basis.

5.1. Concepts and Notations

Recall that [41,42,43] a state ρ A B of H A H B is said to classically correlated (CC) if there exists a rank-1 projective measurement Π = { Π s A Π t B : s [ m ] , t [ n ] } such that
Π ( ρ A B ) : = s = 1 m t = 1 n ( Π s A Π t B ) ρ A B ( Π s A Π t B ) = ρ A B ;
otherwise, ρ A B is said to be quantum correlated (QC). A pure state | ψ is said to be CC (resp. QC) if its density operator | ψ ψ | is CC (resp. QC).
Luo in [41] proved that a state ρ A B of H A H B is CC if and only if it can be represented as
ρ A B = i = 1 n j = 1 m p i j | e i e i | | f j f j | ,
where { p i j } is a PD, { | e i } and { | f j } are some ONBs for H A and H B , respectively. This implies that every CC state is separable while a separable state is not necessarily CC. But a bipartite pure state is CC if and only if it is separable ([48] [Theorem 5.1]).

5.2. Classical Correlation Depending on Basis

Let e A B = { | e i j : i [ d A ] , j [ d B ] } where | e i j = | e i A | e j B ( i [ d A ] , j [ d B ] ) for some ONBs e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively. Then a density operator ρ A B on H A H B has the corresponding density matrix of ρ A B under the basis e A B = e A e B :
ρ e A B A B = [ e i j | ρ A B | e k ] = [ e i A e j B | ρ A B | e k A e B ] ,
which is equal to the matrix representation of the operator
( U A U B ) ρ A B ( U A U B ) : C d A C d B C d A C d B
under the canonical { 0 , 1 } -basis (with m = d A , n = d B )
{ | i A j B } i , j = { | 1 A 1 B , | 1 A 2 B , , | 1 A n B , , | m A 1 B , | m A 2 B , , | m A n B }
for C d A C d B = C d A d B . With this basis, a linear operator X on C d A C d B is usually identified with matrix representation [ i A j B | X | k A B ] . Thus,
ρ e A B A B = ( U A U B ) ρ A B ( U A U B ) ,
where U A and U B are unitary operators given by Equations (8) and (9).
Similarly, when d A = d B = d and | e i j = | e j A | e i B for all i , j [ d ] , we have
ρ e A B A B = S ( U A U B ) ρ A B ( U A U B ) S ,
where S is the swap operator on C d C d .
Using the characterization Equation (15) and Formula (16), we obtain the following.
Theorem 11. 
Let e A B = { | e i j : i [ d A ] , j [ d B ] } where | e i j = | e i A | e j B ( i [ d A ] , j [ d B ] ) for some ONBs e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively. Then
(a) A pure state | ψ A B is CC if and only if its coordinate state | ψ A B e A B is CC.
(b) A density operator ρ A B is CC if and only if its density matrix ρ e A B A B : = [ e i j | ρ A B | e k ] is CC with ( i j , k ) -entry e i j | ρ A B | e k .
Similarly, using the characterization Equation (15) and Formula (17), we obtain the following.
Theorem 12. 
Let d A = d B = d , e A B = { | e i j : i [ d A ] , j [ d B ] } where | e i j = | e j A | e i B ( i [ d A ] , j [ d B ] ) for some ONBs e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively. Then
(a) A pure state | ψ A B is CC if and only if its coordinate state | ψ A B e A B is CC.
(b) A density operator ρ A B is CC if and only if its density matrix ρ e A B A B : = [ e i j | ρ A B | e k ] is CC with ( i j , k ) -entry e i j | ρ A B | e k .
Using Theorems 11 and 12, once can check the following.
Theorem 13. 
Let e A B = { | e i j : i [ d A ] , j [ d B ] } be an orthonormal basis for H A H B and U be fined by Equation (2). Then TFSAE.
(a) | ψ A B is CC if and only if U | ψ A B is CC.
(b) A density operator ρ A B is CC if and only if its density matrix ρ e A B A B : = [ e i j | ρ A B | e k ] is CC with ( i j , k ) -entry e i j | ρ A B | e k .
(c) There exist unitary operators W X : H X C d X ( X = A , B ) such that when d A d B , U = W A W B ; when d A = d B = d , either U = W A W B , or U = S ( W A W B ) , where S : C d C d is the swap operator: S ( | x | y ) = | y | x .
(d) There exist orthonormal bases e A = { | e i A } i = 1 d A and e B = { | e j B } j = 1 d B for H A and H B , respectively, such that when d A d B , | e i j = | e i A | e j B for all i , j ; When d A = d B = d , either | e i j = | e i A | e j B for all i , j , or | e i j = | e j A | e i B for all i , j .

6. Conclusions

Usually, a density operator ρ A B (quantum state ) of a bipartite system A B is represented as a matrix ρ ^ e A B = [ ρ i j ] under a basis e A B = { e i j } i [ d A ] , j [ d B ] for the Hilbert space H A H B of the system A B , called the density matrix of the density operator ρ A B . In this work, we have discussed the relationships between quantum locality and basis, and observed that all density operators and their density matrices under a basis e A B have the same quantum locality if and only if the basis e A B is a product basis of two bases of subsystems. Consequently, different choices of bases may induce different quantum locality; equivalently, different bases define different quantum nonlocality, which we called basis-dependent quantum nonlocality. Also, entangled basis can generate quantum nonlocality of a density matrix from a separable density operator.

Author Contributions

The work of this paper was accomplished by Kaifeng Hu, Zhihua Guo, Huaixin Cao and Ling Lu. Moreover, all authors have read the paper carefully and approved the research contents that were written in the final manuscript.

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Informed consent was obtained from all subjects involved in the study.

Data Availability Statement

Not applicable.

Acknowledgments

This work was supported by the National Natural Science Foundation of China under Grant Nos. 12271325, 11871318, and the Special Plan for Young Top-notch Talent of Shaanxi Province under Grant No. 1503070117.

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. The unitary operator V on C d A C d B .
Figure 1. The unitary operator V on C d A C d B .
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Figure 2. Decomposition of U.
Figure 2. Decomposition of U.
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