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What is Entanglement?

Chon-Fai Kam Chon-Fai Kam is a postdoc of Department of Physics at the State University at Buffalo. His email address is [email protected].    Zhong-Tang Wu Zhong-Tang Wu is a PhD student of Department of Applied Physics at Tunghai University of Taiwan. His email address is [email protected].

1

Entanglement, a puzzle since Einstein’s time, has become increasingly crucial with the rise of quantum computation. But what exactly is it? Entanglement can be precisely defined, but only negatively. As an axiom, the Hilbert space of a composite system of two sub-systems with Hilbert spaces HAH_{A} and HbH_{b}, is given by HAHBH_{A}\otimes H_{B}. If a state of the composite system can be written as

|ψAB=|ψA|ψB,|\psi\rangle_{AB}=|\psi\rangle_{A}\otimes|\psi\rangle_{B}, (1)

it is called a product state. Otherwise it is called an entangled state. Thus, we arrive at Definition 1:

Entangled states are those
which are not product states.\displaystyle\mbox{{which are not product states}}.

But this definition fails to offer a profound understanding of entanglement. To simplify the discussion, we focus on finite dimensional Hilbert spaces. Fixing a basis {|iA}\{|i\rangle_{A}\} for HAH_{A} and a basis {|iB}\{|i\rangle_{B}\} for HBH_{B}, the state |ψAB|\psi_{AB}\rangle can be written as

|ψAB=i,jcij|iA|jB.|\psi\rangle_{AB}=\sum_{i,j}c_{ij}|i\rangle_{A}\otimes|j\rangle_{B}. (2)

In most cases, the state |ψAB|\psi\rangle_{AB} is not a product state. For example, the following four Bell states [nielsen2010quantum] are all not product states

|Φ+AB=12(|0A|0B+|1A|1B),\displaystyle|\Phi_{+}\rangle_{AB}=\frac{1}{\sqrt{2}}\left(|0\rangle_{A}\otimes|0\rangle_{B}+|1\rangle_{A}\otimes|1\rangle_{B}\right), (3a)
|Ψ+AB=12(|0A|1B+|1A|0B),\displaystyle|\Psi_{+}\rangle_{AB}=\frac{1}{\sqrt{2}}\left(|0\rangle_{A}\otimes|1\rangle_{B}+|1\rangle_{A}\otimes|0\rangle_{B}\right), (3b)
|ΦAB12(|0A|0B|1A|1B),\displaystyle|\Phi_{-}\rangle_{AB}\equiv\frac{1}{\sqrt{2}}\left(|0\rangle_{A}\otimes|0\rangle_{B}-|1\rangle_{A}\otimes|1\rangle_{B}\right), (3c)
|ΨAB12(|0A|1B|1A|0B),\displaystyle|\Psi_{-}\rangle_{AB}\equiv\frac{1}{\sqrt{2}}\left(|0\rangle_{A}\otimes|1\rangle_{B}-|1\rangle_{A}\otimes|0\rangle_{B}\right), (3d)

and thus all are entangled according to definition 1.

2

For bipartite systems, one can give a more positive definition of entanglement. Recall that a general bipartite quantum state can be written as

|ψAB=ijcij|iA|jB.|\psi\rangle_{AB}=\sum_{ij}c_{ij}|i\rangle_{A}\otimes|j\rangle_{B}. (4)

The entanglement information is then contained in the matrix M(cij)\textbf{M}\equiv(c_{ij}). One can perform a singular value decomposition M=UDV\textbf{M}=\textbf{U}\textbf{D}\textbf{V}, such that

|ψAB=i=1rλk|ukA|vkB,|\psi\rangle_{AB}=\sum_{i=1}^{r}\lambda_{k}|u_{k}\rangle_{A}\otimes|v_{k}\rangle_{B}, (5)

where |ukAiuik|iA|u_{k}\rangle_{A}\equiv\sum_{i}u_{ik}|i\rangle_{A}, |vkBjvkj|jB|v_{k}\rangle_{B}\equiv\sum_{j}v_{kj}|j\rangle_{B}, and λkdkk\lambda_{k}\equiv d_{kk}. This is called the Schmidt decomposition of |ψAB|\psi\rangle_{AB}, where rr (the rank of the matrix M) is called the Schmidt rank of |ψAB|\psi\rangle_{AB} [bengtsson2017geometry]. Thus, we arrive at Definition 2:

Bipartite entangled states are those
with Schmidt rank greater than one.\displaystyle\mbox{{with Schmidt rank greater than one}}.

In this framework, the Bell states |Φ+AB|\Phi_{+}\rangle_{AB} is considered maximally entangled due to its rank being equal to 22. Unfortunately, Schmidt decomposition does not exist for NN-partite states where NN exceeds 2. However, within the same spirit, it is still possible to express certain multi-partite entangled states. For example, for N=3N=3, the following Greenberger–Horne–Zeilinger (GHZ) state is entangled

|GHZABC\displaystyle|\mbox{GHZ}\rangle_{ABC} 12(|0A|0B|0C\displaystyle\equiv\frac{1}{\sqrt{2}}(|0\rangle_{A}\otimes|0\rangle_{B}\otimes|0\rangle_{C}
+|1A|1B|1C).\displaystyle+|1\rangle_{A}\otimes|1\rangle_{B}\otimes|1\rangle_{C}). (6)

3

For an NN-partite system, the Hilbert space of NN sub-systems with Hilbert spaces H1H_{1}, H2H_{2}, \cdots, HNH_{N}, is given by H1H2HNH_{1}\otimes H_{2}\otimes\cdots\otimes H_{N}. As a matter of fact, through the application of local unitary transformations on each qubit, entanglement cannot be generated from a product state. For example

(U1U2UN)|n1|n2|nN\displaystyle(U_{1}\otimes U_{2}\otimes\cdots\otimes U_{N})|n_{1}\rangle\otimes|n_{2}\rangle\otimes\cdots\otimes|n_{N}\rangle
=|n1|n2|nN\displaystyle=|n_{1}^{\prime}\rangle\otimes|n_{2}^{\prime}\rangle\otimes\cdots\otimes|n_{N}^{\prime}\rangle (7)

is still a product state. Thus, we arrive at Definition 33:

Entangled states are equivalence classes
under the local unitary transformations,
with the exclusion of the class of product states.\displaystyle\mbox{{with the exclusion of the class of product states}}.

Within this framework [grassl1998computing, onishchik2012lie], entanglement theory is the study of the intrinsic geometric properties of multipartite entangled states. To distinguish different entanglement classes under the action of local unitary group G=U1U2UNG=U_{1}\otimes U_{2}\otimes\cdots\otimes U_{N}, an entanglement invariant becomes necessary [miyake2003classification]. Recall that for the bipartite case, one can use the Schmidt rank to distinguish entangled states from product states. Hence, for a bipartite qubit state |ψAB=i,j=01cij|iA|jB|\psi\rangle_{AB}=\sum_{i,j=0}^{1}c_{ij}|i\rangle_{A}\otimes|j\rangle_{B} with a Hilbert space given by 22\mathbb{C}^{2}\otimes\mathbb{C}^{2}, the determinant of the matrix M=(cij)\textbf{M}=(c_{ij}), defined as detM=detD=λ1λ2\det\textbf{M}=\det\textbf{D}=\lambda_{1}\lambda_{2} serves as an entanglement invariant. Here, M is invariant under SL(2,)2\mbox{SL}(2,\mathbb{C})^{\otimes 2} transformations, and thus invariant under SU(2,)2\mbox{SU}(2,\mathbb{C})^{\otimes 2} transformations. Additionally, detM\det\textbf{M} vanishes when the matrix M is not full rank. In other words, a bipartite qubit state |ψAB|\psi\rangle_{AB} is a product state only when the discriminant detM=c00c11c01c10\det\textbf{M}=c_{00}c_{11}-c_{01}c_{10} vanishes. For example, a direct computation yields

det(|Φ+AB)=1,\det(|\Phi_{+}\rangle_{AB})=1, (8)

indicating that the Bell state |Φ+AB|\Phi_{+}\rangle_{AB} is entangled. It is noteworthy that the Bell states |ΦAB|\Phi_{-}\rangle_{AB}, |Ψ+AB|\Psi_{+}\rangle_{AB} and |ΨAB|\Psi_{-}\rangle_{AB} can be obtained from |Φ+AB|\Phi_{+}\rangle_{AB} by applying Pauli ZZ and XX gates exclusively on the first qubit

|ΦAB=(ZI)|Φ+AB,\displaystyle|\Phi_{-}\rangle_{AB}=(Z\otimes I)|\Phi_{+}\rangle_{AB}, (9a)
|Ψ+AB=(XI)|Φ+AB,\displaystyle|\Psi_{+}\rangle_{AB}=(X\otimes I)|\Phi_{+}\rangle_{AB}, (9b)
|ΨAB=(ZXI)|Φ+AB.\displaystyle|\Psi_{-}\rangle_{AB}=(ZX\otimes I)|\Phi_{+}\rangle_{AB}. (9c)

This demonstrates that all four Bell states are in the same entanglement class under the action of local unitary transformations. Notice that since det(|Φ+AB)=det(|Ψ+AB)=1\det(|\Phi_{+}\rangle_{AB})=\det(|\Psi_{+}\rangle_{AB})=1 and det(|ΦAB)=det(|ΨAB)=1\det(|\Phi_{-}\rangle_{AB})=\det(|\Psi_{-}\rangle_{AB})=-1, the square of the discriminant as a polynomial function of the coefficients cijc_{ij} serves as a more suitable measure of entanglement.

4

For tri-partite qubit states, there exists a similar entanglement measure called hyper-determinant. For a tri-partite qubit state |ψABC=i,j,k=01cijk|iA|jB|kC|\psi\rangle_{ABC}=\sum_{i,j,k=0}^{1}c_{ijk}|i\rangle_{A}\otimes|j\rangle_{B}\otimes|k\rangle_{C}, the hyperdeterminant is defined by

Det(|ψABC)c0002c1112+c0012c1102+c0102c1012\displaystyle\mbox{Det}(|\psi\rangle_{ABC})\equiv c^{2}_{000}c^{2}_{111}+c^{2}_{001}c^{2}_{110}+c^{2}_{010}c^{2}_{101}
+c1002c01122c000c001c110c1112c000c010c101c111\displaystyle+c^{2}_{100}c^{2}_{011}-2c_{000}c_{001}c_{110}c_{111}-2c_{000}c_{010}c_{101}c_{111}
2c000c011c100c1112c001c010c101c110\displaystyle-2c_{000}c_{011}c_{100}c_{111}-2c_{001}c_{010}c_{101}c_{110}
2c001c011c110c1002c010c011c101c100\displaystyle-2c_{001}c_{011}c_{110}c_{100}-2c_{010}c_{011}c_{101}c_{100}
+4c000c011c101c110+4c001c010c100c111.\displaystyle+4c_{000}c_{011}c_{101}c_{110}+4c_{001}c_{010}c_{100}c_{111}. (10)

The hyper-determinant is invariant under SL(2,)3\mbox{SL}(2,\mathbb{C})^{\otimes 3} transformations, and thus invariant under SU(2,)3\mbox{SU}(2,\mathbb{C})^{\otimes 3} transformations. The utilization of the hyper-determinant demonstrates that the WW state, characterized as

|WABC13(|0A|0B|1C\displaystyle|W\rangle_{ABC}\equiv\frac{1}{\sqrt{3}}(|0\rangle_{A}\otimes|0\rangle_{B}\otimes|1\rangle_{C}
+|0A|1B|0C+|1A|0B|0C)\displaystyle+|0\rangle_{A}\otimes|1\rangle_{B}\otimes|0\rangle_{C}+|1\rangle_{A}\otimes|0\rangle_{B}\otimes|0\rangle_{C}) (11)

is in a distinct entanglement class under the action of local unitary group, compared to the GHZ state. A direct computation yields

Det(|GHZABC)=14,Det(|WABC)=0.\mbox{Det}(|\mbox{GHZ}\rangle_{ABC})=\frac{1}{4},\mbox{Det}(|W\rangle_{ABC})=0. (12)

Thus, the WW and GHZ states belong to different entanglement classes according to definition 3.

5

The discussion is not necessarily constrained to qubits. One can also consider multi-partite qutrit states. For a tri-partite qutrit state |ψABCi,j,k=1,2,3cijk|iA|jB|kC|\psi\rangle_{ABC}\equiv\sum_{i,j,k=1,2,3}c_{ijk}|i\rangle_{A}\otimes|j\rangle_{B}\otimes|k\rangle_{C}, one can derive Nurmiev’s normal form [nurmiev2000orbits] through SU(3,)3\mbox{SU}(3,\mathbb{C})^{\otimes 3} transformations

|ψ¯ABC=a1(|1A|1B|1C+|2A|2B|2C\displaystyle\overline{|\psi\rangle}_{ABC}=a_{1}(|1\rangle_{A}\otimes|1\rangle_{B}\otimes|1\rangle_{C}+|2\rangle_{A}\otimes|2\rangle_{B}\otimes|2\rangle_{C}
+|3A|3B|3C)+a2(|1A|2B|3C\displaystyle+|3\rangle_{A}\otimes|3\rangle_{B}\otimes|3\rangle_{C})+a_{2}(|1\rangle_{A}\otimes|2\rangle_{B}\otimes|3\rangle_{C}
+|2A|3B|1C+|3A|1B|2C)\displaystyle+|2\rangle_{A}\otimes|3\rangle_{B}\otimes|1\rangle_{C}+|3\rangle_{A}\otimes|1\rangle_{B}\otimes|2\rangle_{C})
+a3(|1A|3B|2C+|2A|1B|3C)\displaystyle+a_{3}(|1\rangle_{A}\otimes|3\rangle_{B}\otimes|2\rangle_{C}+|2\rangle_{A}\otimes|1\rangle_{B}\otimes|3\rangle_{C})
+|3A|2B|1C).\displaystyle+|3\rangle_{A}\otimes|2\rangle_{B}\otimes|1\rangle_{C}). (13)

The entanglement classes are determined by three fundamental invariants I6I_{6}, I9I_{9} and I12I_{12}, which can be explicitly expressed as [olver1999classical]

I6\displaystyle I_{6} =a16+a26+a3610(a13a23+a13a33+a23a33),\displaystyle=a_{1}^{6}+a_{2}^{6}+a_{3}^{6}-10(a_{1}^{3}a_{2}^{3}+a_{1}^{3}a_{3}^{3}+a_{2}^{3}a_{3}^{3}), (14a)
I9\displaystyle I_{9} =(a13a23)(a13a33)(a23a33),\displaystyle=-(a_{1}^{3}-a_{2}^{3})(a_{1}^{3}-a_{3}^{3})(a_{2}^{3}-a_{3}^{3}), (14b)
I12\displaystyle I_{12} =(a13+a23+a33)[(a13+a23+a33)3+(6a1a2a3)3].\displaystyle=-(a_{1}^{3}+a_{2}^{3}+a_{3}^{3})[(a_{1}^{3}+a_{2}^{3}+a_{3}^{3})^{3}+(6a_{1}a_{2}a_{3})^{3}]. (14c)

The invariants I6I_{6} and I12I_{12} are determined up to nonzero scalar multiples, whereas I12I_{12} is solely determined up to a scalar multiple of I62I_{6}^{2}. Various conventions exist regarding the representation of I12I_{12}. For example, the Bremner invariant, denoted as J12J_{12}, is related to I6I_{6} and I12I_{12} by I12I62=24J12-I_{12}-I_{6}^{2}=24J_{12}. As such, the explicit form of the 3×3×33\times 3\times 3 hyperdeterminant is given by [bremner20143]

Δ=I63I92I62J122+36I6I92J12+108I9432J123.\Delta=I_{6}^{3}I_{9}^{2}-I_{6}^{2}J_{12}^{2}+36I_{6}I_{9}^{2}J_{12}+108I_{9}^{4}-32J_{12}^{3}. (15)

For instance, the following tri-partite qutrit state is maximally entangled when both AA and BB are non-zero

|ϕ\displaystyle|\phi ABCα(|3A|2B|1C+|1A|2B|3C)\displaystyle\rangle_{ABC}\equiv\alpha(|3\rangle_{A}\otimes|2\rangle_{B}\otimes|1\rangle_{C}+|1\rangle_{A}\otimes|2\rangle_{B}\otimes|3\rangle_{C})
+β(|3A|1B|2C+|1A|3B|2C\displaystyle+\beta(|3\rangle_{A}\otimes|1\rangle_{B}\otimes|2\rangle_{C}+|1\rangle_{A}\otimes|3\rangle_{B}\otimes|2\rangle_{C}
+|2A|3B|1C+|2A|1B|3C).\displaystyle+|2\rangle_{A}\otimes|3\rangle_{B}\otimes|1\rangle_{C}+|2\rangle_{A}\otimes|1\rangle_{B}\otimes|3\rangle_{C}). (16)

The reason behind this is that the three fundamental invariants I6I_{6}, I9I_{9} and I12I_{12} for |ψ0|\psi_{0}\rangle are I6=8α2β4I_{6}=-8\alpha^{2}\beta^{4} and I9=I12=0I_{9}=I_{12}=0. Thus, the hyperdeterminant Δ\Delta for |ϕABC|\phi\rangle_{ABC} has the form

Δ(|ϕABC)=11728I66=409627(αβ2)12,\Delta(|\phi\rangle_{ABC})=\frac{1}{1728}I_{6}^{6}=\frac{4096}{27}(\alpha\beta^{2})^{12}, (17)

which is non-zero when both α\alpha and β\beta are non-zero.

6

For a general multipartite entangled state, if one can identify all invariants under local unitary transformations, the task of classifying entangled states is accomplished [bennett2000exact]. But this turns out to be an extremely difficult task. Fortunately, for multipartite entangled state with certain symmetries, the task is greatly simplified. Notice that all previously discussed important entangled states, like Bell states, GHZ states and WW states, are all symmetric with respect to permutation of qubits. In general, NN-partite permutation symmetric states can be defined as

|ψ=1N!ANσSN|nσ(1)|nσ(N),|\psi\rangle=\frac{1}{\sqrt{N!A_{N}}}\sum_{\sigma\in S_{N}}|n_{\sigma(1)}\rangle\otimes\cdots\otimes|n_{\sigma(N)}\rangle, (18)
Refer to caption
(a) GHZ-like states
Refer to caption
(b) W-like States
Figure 1: Majorana representation for tri-partite entangled states [kam2020three].

where SNS_{N} is the symmetric group on NN letters, and ANA_{N} is a normalization factor. Remarkably, these types of multipartite entangled state which are symmetric respect to permutation of qubits, can be represented geometrically by an assembly of NN unordered points on a unit sphere. The reason is simple: a permutation symmetric state, i.e., σ(|ψ)=|ψ\sigma(|\psi\rangle)=|\psi\rangle for arbitrary σSn\sigma\in S_{n}, is homeomorphic to an NN-fold symmetric tensor product of spheres. In physics literature, this is called the Majorana representation, where the unordered points are referred to as Majorana stars [ribeiro2011entanglement]. In Fig. 1, we illustrate the Majorana representation for GHZ-like states and WW-like states, while the former has three distinct stars and the later has only two distinct stars. Thus, we arrive at Definition 4:

For those states which are invariant
under permutation of qubits,\displaystyle\mbox{{under permutation of qubits}},
the entangled classes are determined by
the number of distinct Majorana Stars.\displaystyle\mbox{{the number of distinct Majorana Stars}}.

When Majorana stars undergo stereographic projection onto the complex plane, the degenerate patterns the stars display align with the nature of roots of a polynomial termed the Majorana polynomial. A non-zero discriminant of the Majorana polynomial corresponds to a maximally entangled state.

The state with the fewest number of stars is called the coherent state [kam2023coherent], wherein all NN stars degenerate into a single star. It represents the most classical state without any entanglement. In this regard, there exists an onion structure for permutation symmetric states:

spin-1 coherent states Bell states,\displaystyle\prec\mbox{Bell states},
spin-32\frac{3}{2} coherent states W statesGHZ states,\displaystyle\prec\mbox{$W$ states}\prec\mbox{GHZ states},
\displaystyle\vdots\>\>\>\>\>\>\>\>\>\> \displaystyle\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\>\vdots
spin-N2\frac{N}{2} coherent states N-qubit GHZ states.\displaystyle\prec\cdots\prec\mbox{$N$-qubit GHZ states}. (19)

The above sets up a partial order filtering that always begins with coherent states, which are the most classical, and ends with GHZ states, renowned for being maximally entangled. In this regard, for permutation symmetric states, the problem of classifying entanglement transforms into the spherical design problem, also known as the Thomson problem [bengtsson2017geometry].

To conclude, the four definitions of entangled states discussed here are all interconnected. The third definition represents an advancement over the first, as it encompasses a wider range of scenarios, albeit with computational complexities. Additionally, the fourth definition essentially restates the second one when specifically addresses bipartite symmetric states.

References