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I. INTRODUCTION
The modern development of the quantum computing technique implies various extensions of its foundational concepts [1–3]. One of the main problems in the physical realization of quantumcomputersis presence of errors, which implies that it is desirable that quantum computations be provided with error correction, or that ways be found to make the states more stable, which leads to the concept of topological quantum computation (for reviews, see, e.g., [4–6], and references therein). In the Turaev approach [7], link invariants can be obtained from the solutions of the constant Yang-Baxter equation (the braid equation). It was realized that the topological entanglement of knots and links is deeply connected with quantum entanglement [8, 9]. Indeed, if the solutions to the constant Yang-Baxter equation [10] (Yang-Baxter operators/maps [11, 12]) are interpreted as a special class of quantum gate, namely braiding quantum gates [13, 14], then the inclusion of non-entangling gates does not change the relevant topological invariants [15, 16]. For further properties and applications of braiding quantum gates, see [17–20]. In this paper we obtain and study the solutions to the higher arity (polyadic) braid equations introduced in [21, 22], as a polyadic generalization of the constant Yang-Baxter equation (which is considerably different from the generalized Yang-Baxter equation of [23–26]). We introduce special classes of matrices (star and circle types), to which most of the solutions belong, and find that the so-called magic matrices [18, 27, 28] belong to the star class. We investigate their general non-trivial group properties and polyadic generalizations. We then consider the invertible and non-invertible matrix solutions to the higher braid equations as the corresponding higher braiding gates acting on multi-qubit states. It is important that multi-qubit entanglement can speed up quantum key distribution [29] and accelerate various algorithms [30]. As an example, we have made detailed computations for the ternary braiding gates as solutions to the ternary braid equations [21, 22]. A particular solution to the n-ary braid equation is also presented. It is shown, that for each multi-qubit state there exist higher braiding gates which are not entangling, and the concrete relations for that are obtained, which can allow us to build non-entangling networks.
II. YANG-BAXTER OPERATORS
Recall here [9, 13] the standard construction of the special kind of gates we will consider, the braiding gates, in terms of solutions to the constant Yang-Baxter equation [10] (called also algebraic Yang-Baxter equation [31]), or the (binary) braid equation [21].
A. Yang-Baxter maps and braid group
First we consider a general abstract construction of the (binary) braid equation. Let V be a vector space over a field K and the mapping CV2 : V V V V, where = K is the tensor product over K. A linear operator (braid operator) CV2 is called a Yang-Baxter operator⊗ →(denoted⊗ by R in⊗ [13]⊗ and by B in [10]) or Yang-Baxter map [12] (denoted by F in [11]), if it satisfies the braid equation [32–34]
(C 2 id ) (id C 2 ) (C 2 id ) = (id C 2 ) (C 2 id ) (id C 2 ) , (2.1) V ⊗ V ◦ V ⊗ V ◦ V ⊗ V V ⊗ V ◦ V ⊗ V ◦ V ⊗ V where idV : V V, is the identity operator in V. The connection of CV2 with the R-matrix R is given by CV2 = τ R, where τ is the flip operation→ [10, 11, 32]. ◦ Let us introduce the operators A : V V V V V V by 1,2 ⊗ ⊗ → ⊗ ⊗ A =C 2 id , A = id C 2 , (2.2) 1 V ⊗ V 2 V ⊗ V It follows from (2.1) that
A A A = A A A . (2.3) 1 ◦ 2 ◦ 1 2 ◦ 1 ◦ 2
2 1 1 1 If CV is invertible, then CV−2 is also the Yang-Baxter map with A1− and A2− . Therefore, the operators Ai represent the braid group = e, σ , σ σ σ σ = σ σ σ by the mapping π as B3 { 1 2 | 1 2 1 2 1 2} 3 π3 π3 π3 π3 End (V V V) , σ A , σ A , e id . (2.4) B3 −→ ⊗ ⊗ 1 7→ 1 2 7→ 2 7→ V
The representation πm of the braid group with m strands
σiσi+1σi = σi+1σiσi+1, i =1,...,m 1, m = e, σ1,...,σm 1 − (2.5) B { − σiσj = σj σi, i j 2, | − |≥
3
m m can be obtained using operators A (m):V⊗ V⊗ analogous to (2.2) i → i 1 m i 1 − − − m A (m)= id ... id C 2 id ... id , A (m) = (id )⊗ , i =1,...,m 1, (2.6) i V ⊗ ⊗ V ⊗ V ⊗ V ⊗ V 0 V − z }| m { z }| { by the mapping π : EndV⊗ in the following way m Bm →
πm (σi) = Ai (m) , πm (e) = A0 (m) . (2.7) In this notation (2.2) is A = A (2), i =1, 2, and therefore (2.3) represents by (2.4). i i B3
B. Constant matrix solutions to the Yang-Baxter equation
Consider next a concrete version of the vector space V which is used in the quantum computation, a d-dimensional euclidean vector space Vd over complex numbers C with a basis ei , i = 1,...,d. A linear operator Vd Vd is given by a complex { } → 2 2 d d matrix, the identity operator id becomes the identity d d matrix I , and the Yang-Baxter map C 2 is a d d matrix × V × d V × Cd2 (denoted by R in [31]) satisfying the matrix algebraic Yang-Baxter equation
(C 2 I ) (I C 2 ) (C 2 I ) = (I C 2 ) (C 2 I ) (I C 2 ) , (2.8) d ⊗ d d ⊗ d d ⊗ d d ⊗ d d ⊗ d d ⊗ d being an equality between two matrices of size d3 d3. We use the unified notations which can be straightforwardly generalized for higher braid operators. In components ×
d ′ ′ j1j2 2 ′ ′ Cd (ei1 ei2 )= ci1i2 ej1 ej2 , (2.9) ◦ ⊗ ′ ′ · ⊗ j1X,j2=1 the Yang-Baxter equation (2.8) has the shape (where summing is by primed indices)
d ′ ′ ′ d ′ ′ ′ j1j2 j3k3 k1k2 l2l3 k1l1 k2k3 k1k2k3 c c ′ c ′ ′ = c c ′ c ′ ′ q . (2.10) i1i2 j2i3 j1j3 i2i3 i1l2 l1l3 i1i2i3 ′ ′ ′ · · ′ ′ ′ · · ≡ j1,jX2,j3=1 l1,lX2,l3=1 4 6 The system (2.10) is highly overdetermined, because the matrix Cd2 contains d unknown entries, while there are d cubic polynomial equations for them. So for d = 2 we have 64 equations for 16 unknowns, while for d = 3 there are 729 equations 2 for the 81 unknown entries of Cd2 . The unitarity of Cd2 imposes a further d quadratic equations, and so for d = 2 we have in total 68 equations for 16 unknowns. This makes the direct discovery of solutions for the matrix Yang-Baxter equation (2.10) very cumbersome. Nevertheless, using a conjugation classes method, the unitary solutions and their classification for d = 2 were presented in [31]. In the standard matrix form (2.9) can be presented by introducing the 4-dimensional vector space V˜4 = V V with the natural ˜ ⊗ ˜ ˜ ˜ basis e˜k˜ = e1 e1,e1 e2,e2 e1,e2 e2 , where k = 1,..., 8 is a cumulative index. The linear operator C4 : V4 V4 { ⊗ ⊗ ⊗ ⊗ } 4 → corresponding to (2.9) is given by 4 4 matrix c˜ ˜ as C˜ e˜ = c˜ ˜ e˜˜. The operators (2.2) become two 8 8 matrices × ˜ıj 4 ◦ ˜ı ˜j=1 ˜ıj · j × A˜ as 1,2 P A˜ =˜c I , A˜ = I c,˜ (2.11) 1 ⊗K 2 2 2 ⊗K where K is the Kronecker product of matrices and I2 is the 2 2 identity matrix. In this notation (which is universal and also used for⊗ higher braid equations) the operator binary braid equations× (3.7) become a single matrix equation
A˜1A˜2A˜1 = A˜2A˜1A˜2, (2.12) which we call the matrix binary braid equation (and also the constant Yang-Baxter equation [31]). In component form (2.12) is a highly overdetermined system of 64 cubic equations for 16 unknowns, the entries of c˜. The matrix equation (2.12) has the following “gauge invariance”, which allows a classification of Yang-Baxter maps [35]. Introduce an invertible operator Q : V V in the two-dimensional vector space V Vd=2. In the basis e1,e2 its 2 2 2 → ≡ { } × matrix q is given by Q e = q e . In the natural 4-dimensional basis e˜˜ the tensor product of operators Q Q is ◦ i j=1 ij · j k ⊗ presented by the Kronecker product of matrices q˜4 = q K q. Ifthe 4 4 matrix c˜is a fixed solution to the Yang-Baxter equation (2.12), then the family of solutionsP c˜(q) corresponding⊗ to the invertible× 2 2 matrix q is the conjugation of c˜ by q˜ such that × 4 1 1 1 c˜(q)=˜q c˜q˜− = (q q)˜c q− q− , (2.13) 4 4 ⊗K ⊗K 4 which follows from conjugating (2.12) by q K q and using (2.11). If we include the obvious invariance of (2.12) with respect to an overall factor t C, the general family⊗ of solutions becomes (cf. the Yang-Baxter equation [35]) ∈ 1 1 1 c˜(q,t)= tq˜ c˜q˜− = t (q q)˜c q− q− . (2.14) 4 4 ⊗K ⊗K It follows from (2.13) that the matrix q GL (2, C) is defined up to a complex non-zero factor. In this case we can put ∈ a 1 q = , (2.15) c d and the manifest form of q˜4 is
a2 a a 1 acad c d q˜ = . (2.16) 4 ac c ad d 2 2 c cd cd d ⋆ ⋆ The matrix q˜4 q˜4 (where represents Hermitian conjugation) is diagonal (this case is important in a further classification similar to the binary one [31]), when the condition
c = a/d∗ (2.17) − holds, and so the matrix q takes the special form (depending on 2 complex parameters)
a 1 q = . (2.18) a/d∗ d −
We call two solutions c˜1 and c˜2 of the constant Yang-Baxter equation (2.12) q-conjugated, if
c˜1q˜4 =q ˜4c˜2, (2.19) and we will not distinguish between them. The q-conjugation in the form (2.19) does not require the invertibility of the matrix q, and therefore the solutions of different ranks (or invertible and not invertible) can be q-conjugated (for the invertible case, see [35–37]). The matrix equation (2.12) does not imply the invertibility of solutions, i.e. matrices c˜ being of full rank (in the binary Yang- Baxter case of rank 4 and d =2). Therefore, below we introduce in a unified way invertible and non-invertible solutions to the matrix Yang-Baxter equation (2.10) for any rank of the corresponding matrices.
C. Partial identity and unitarity
To be as close as possible to the invertible case, we introduce “non-invertible analogs” of identity and unitarity. Let M be a diagonal n n matrix of rank r n, and therefore with n r zeroes on the diagonal. If the other diagonal elements are units, × ≤ − such a diagonal M can be reduced by row operations to a block matrix, being a direct sum of the identity matrix Ir r and the r × n r − (block) zero matrix Z(n r) (n r). We call such a diagonal matrix a block r-partial identity In (r) = diag 1,... 1,0,..., 0 , − × − (shuffle) z }| { z }| { and without the block reduction—a shuffle r-partial identity In (r) (these are connected by conjugation). We will use the term partial identity and I (r) to denote any matrix of this form. Obviously, with the full rank r = n we have I (n) I, n n ≡ n where In is the identity n n matrix. As with the invertible case and identities, the partial identities (of the corresponding form) are trivial solutions of the× Yang-Baxter equation. If a matrix M = M (r) of size n n and rank r satisfies the following r-partial unitarity condition × ⋆ (1) M (r) M (r)= In (r) , (2.20) ⋆ (2) M (r) M (r) = In (r) , (2.21)
⋆ (1) (2) where M (r) is the conjugate-transposed matrix and In (r), In (r) are partial identities (of any kind, they can be different), (1) (2) then M (r) is called a r-partial unitary matrix. In the case, when In (r) = In (r), the matrix M (r) is called normal. If ⋆ M (r) = M (r), then it is called r-partial self-adjoint. In the case of full rank r = n, the conditions (2.20)–(2.21) become 5 ordinary unitarity, and M (n) becomes an unitary (and normal) matrix, while a r-partial self-adjoint matrix becomes a self- adjoint matrix or Hermitian matrix. As an example, we consider a 4 4 matrix of rank 3 × 0 000 0 eiβ 0 0 M (3) = , α,β,γ R, (2.22) 0 00 eiγ ∈ eiα 0 0 0 which satisfies the 3-partial unitarity conditions (2.20)–(2.21) with two different 3-partial identities on the r.h.s.
1000 0000 ⋆ 0100 (1) (2) 0100 ⋆ M (3) M (3) = = I (3) = I (3) = = M (3) M (3) . (2.23) 0000 4 6 4 0010 0001 0001 For a non-invertible matrix M (r) one can define a pseudoinverse M (r)+ (or the Moore-Penrose inverse) [38] by
M (r) M (r)+ M (r)= M (r) ,M (r)+ M (r) M (r)+ = M (r)+ , (2.24) and M (r) M (r)+, M (r)+ M (r) are Hermitian. In the case of (2.22) the partial unitary matrix M (3) coincides with its pseudoinverse
⋆ M (3) = M (3)+ , (2.25)
⋆ 1 which is similar to the standard unitarity Minv = Minv− for an invertible matrix Minv. It is important that (2.22) is a solution of the matrix Yang-Baxter equation (2.12), and so is an example of a non-invertible Yang-Baxter map. If only the first (second) of the conditions (2.20)–(2.21) holds, we call such M (r) a left (right) r-partial unitary matrix. An example of such a non-invertible Yang-Baxter map of rank 2 is the left 2-partial unitary matrix
0 0 0 eiα iβ 1 0 e 0 0 R M (2) = iβ , α,β , (2.26) √2 0 e 0 0 ∈ 0 0 0 eiβ which satisfies (2.20), but not (2.21), and so M (2) is not normal
i(α β) 0000 1 00 e − ⋆ 0100 0 11 0 ⋆ M (2) M (2) = = = M (2) M (2) . (2.27) 0000 6 0 11 0 i(β α) 0001 e − 00 1 ⋆ Nevertheless, the property (2.25) still holds and M (2) = M (2)+.
D. Permutation and parameter-permutation 4-vertex Yang-Baxter maps
The system (2.12) with respect to all 16 variables is too cumbersome for direct solution. The classification of all solutions can only be accomplished in special cases, e.g. for matrices over finite fields [35] or for fewer than 16 vertices. Here we will start from 4-vertex permutation and parameter-permutation matrix solutions and investigate their group structure. It was shown [13, 31] that the special 8-vertex solutions to the Yang-Baxter equation are most important for further applications including braiding gates. We will therefore study the 8-vertex solutions in the most general way: over C and in various configurations, invertible and not invertible, and also consider their group structure. First, we introduce the permutation Yang-Baxter maps which are presented by the permutation matrices (binary matrices with a single 1 in each row and column), i.e. 4-vertex solutions. In total, there are 64 permutation matrices of size 4 4, while only × 6
4 of them have the full rank 4 and simultaneously satisfy the Yang-Baxter equation (2.12). These are the following
1000 0001 0010 0100 trc ˜ =2, detc ˜ = 1, c˜perm = , , − (2.28) bisymm 0100 0010 eigenvalues: 1 [2] , 1 [2] , { } {− } 0001 1000 0100 0010 0001 1000 trc ˜ =0, detc ˜ = 1, c˜perm = , , (2.29) 90symm 1000 0001 eigenvalues: 1, i, 1−, i. − − 0010 0100 Here and next we list eigenvalues to understand which matrices are conjugated, and after that, if and only if the conjugation matrix is of the form (2.16), then such solutions to the Yang-Baxter equation (2.12) coincide. The traces are important in the construction of corresponding link invariants [7] and local invariants [39, 40], and determinants are connected with the concurrence [41, 42]. Note that the first matrix in (2.28) is the SWAP quantum gate [1]. To understand symmetry properties of (2.28)–(2.29), we introduce the so called reverse matrix J J of size n n by ≡ n × (Jn) = δi,n+1 i. For n =4 it is ij −
0001 0010 J = . (2.30) 4 0100 1000
For any n n matrix M Mn the matrix JM is the matrix M reflected vertically, and the product MJ is M reflected horizontally. In× addition to the≡ standard symmetric matrix satisfying M = M T (T is the transposition), one can introduce
M is persymmetric, if JM = (JM)T , (2.31) T M is 90◦-symmetric, if M = JM. (2.32)
Thus, a persymmetric matrix is symmetric with respect to the minor diagonal, while a 90◦-symmetric matrix is symmetric under 90◦-rotations. A bisymmetric matrix is symmetric and persymmetric simultaneously. In this notation, the first family of the permutation solutions (2.28) are bisymmetric, but not 90◦-symmetric, while the second family of the solutions (2.29) are, oppositely, 90◦-symmetric, but not symmetric and not persymmetric (which explains their notation). In the next step, we define the corresponding parameter-permutation solutions replacing the units in (2.28) by parameters. We found the following four 4-vertex solutions to the Yang-Baxter equation (2.12) over C
x 0 0 0 0 0 0 y trc ˜ = x + t, 0 0 y 0 0 x 0 0 c˜perm,star (x,y,z,t)= , , det˜c = xyzt, x,y,z,t =0, (2.33) rank=4 0 z 0 0 0 0 t 0 − 6 eigenvalues: x, t, √yz, √yz, 0 00 t z 0 0 0 − 0 0 x 0 0 x 0 0 trc ˜ =0, y 0 0 0 0 0 0 x c˜perm,circ (x, y)= , , detc ˜ = x2y2, x,y =0, (2.34) rank=4 0 0 0 x y 0 0 0 − 6 eigenvalues: √xy, √xy,i√xy, i√xy. 0 y 0 0 0 0 y 0 − − The first pair of solutions (2.33) correspond to the bi-symmetric permutation matrices (2.28), and we call them star-like solutions, while the second two solutions (2.34) correspond to the 90◦-symmetric matrices (2.28) which are called circle-like solutions. The first (second) star-like solution in (2.33) with y = z (x = t) becomes symmetric (persymmetric), while on the other hand with x = t (y = z) it becomes persymmetric (symmetric). They become bisymmetric parameter-permutation solutions if all the parameters are equal x = y = z = t. The circle-like solutions (2.34) are 90◦-symmetric when x = y. Using q-conjugation (2.14) one can next get families of solutions depending from the entries of q, the additional complex parameters in (2.15). 7
E. Group structure of 4-vertex and 8-vertex matrices
Let us analyze the group structure of 4-vertex matrices (2.33)–(2.34) with respect to matrix multiplication, i.e. which kinds of subgroups in GL(4, C) they can form. For this we introduce four 4-vertex 4 4 matrices over C: two star-like matrices × x 0 0 0 0 0 0 y tr N = x + t, 0 0 y 0 0 x 0 0 N = , N = , det N = xyzt, x,y,z,t =0, (2.35) star1 0 z 0 0 star2 0 0 t 0 − 6 eigenvalues: x, t, √yz, √yz, 0 0 0 t z 0 00 − and two circle-like matrices 0 0 x 0 0 x 0 0 tr N =0, y 0 0 0 0 0 0 y N = ,N = , det N = xyzt, x,y,z,t =0, . (2.36) circ1 0 0 0 z circ2 z 0 00 eigenvalues: √4 xyzt,− √4 xyzt,i√4 xyzt,6 √4 xyzt, 0 t 0 0 0 0 t 0 − − Denoting the corresponding sets by Nstar1,2 = Nstar1,2 and Ncirc1,2 = Ncirc1,2 , these do not intersect and are closed with respect to the following multiplications { } { }
Nstar1Nstar1Nstar1 = Nstar1, (2.37)
Nstar2Nstar2Nstar2 = Nstar2, (2.38)
Ncirc1Ncirc1Ncirc1Ncirc1Ncirc1 = Ncirc1, (2.39)
Ncirc2Ncirc2Ncirc2Ncirc2Ncirc2 = Ncirc2. (2.40)
Note that there are no closed binary multiplications among the sets of 4-vertex matrices (2.35)–(2.36). To give a proper groupinterpretationof (2.37)–(2.40), we introduce a k-ary (polyadic) general linear semigroup GLS[k] (n, C)= [k] [k] Mfull µ , where Mfull = Mn n is the set of n n matrices over C and µ is an ordinary product of k matrices. The | { × } × full semigroup [k] C is derived in the sense that its product can be obtained by repeating the binary products which GLS (n, ) are (binary) closed at each step. However, n n matrices of special shape can form k-ary subsemigroups of GLS[k] (n, C) which can be closed with respect to the product× of at minimum k matrices, but not of 2 matrices, and we call such semigroups k-non-derived. Moreover, we have for the sets Nstar1,2 and Ncirc1,2
M = N N N N , N N N N = ∅. (2.41) full star1 ∪ star2 ∪ circ1 ∪ circ2 star1 ∩ star2 ∩ circ1 ∩ circ2 A simple example of a 3-nonderived subsemigroup of the full semigroup GLS[k] (n, C) is the set of antidiagonal matrices [3] Madiag = Madiag (having nonzero elements on the minor diagonal only): the product µ of 3 matrices from Madiag is closed, { } [3] [3] [3] and therefore Madiag is a subsemigroup = Madiag µ of the full ternary general linear semigroup GLS (n, C) with Sadiag | the multiplication µ[3] as the ordinary triple matrix product. 1 In the theory of polyadic groups [43] an analog of the binary inverse M − is given by the querelement, which is denoted by M¯ and in the matrix k-ary case is defined by
k 1 − M...MM¯ = M, (2.42) z }| { where M¯ can be on any place. If each element of the k-ary semigroup GLS[k] (n, C) (or its subsemigroup) has its querelement M¯ , then this semigroup is a k-ary general linear group GL[k] (n, C). In the set of n n matrices the binary (ordinary) product is defined (even it is not closed), and for invertible matrices we × 1 formally determine the standard inverse M − , but for arity k 4 it does not coincide with the querelement M¯ , because, as follows from (2.42) and cancellativity in C that ≥
2 k M¯ = M − . (2.43)
[k] [k] The k-ary (polyadic) identity In in GLS (n, C) is defined by
k 1 − [k] [k] In ...In M = M, (2.44) z }| { 8 which holds when M in the l.h.s. is on any place. If M is only on one or another side (but not in the middle places) in (2.44), [k] [k] C [3] In is called left (right) polyadic identity. For instance, in the subsemigroup (in GLS (n, )) of antidiagonal matrices adiag [3] S the ternary identity In can be chosen as the n n reverse matrix (2.30) having units on the minor diagonal, while the ordinary [3] × [k] n n unit matrix I is not in . It follows from (2.44), that for matrices over C the (left, right) polyadic identity In is × n Sadiag
k 1 [k] − In = In, (2.45) [k] [k] which means that for the ordinary matrix product In is a (k 1)-root of I (or In is a reflection of (k 1) degree), while both − n − sides cannot belong to a subsemigroup [k] of GLS[k] (n, C) under consideration (as in [3] ). As the solutions of (2.45) are not S Sadiag [k] [k] unique, there can be many k-ary identities in a k-ary matrix semigroup. We denote the set of k-ary identities by In = In . [3] [3] In the case of the ternary identity In can be chosen as any of the n n reverse matrices (2.30) with unit complex numbersn o Sadiag × iαj e , j = 1,...,n on the minor diagonal, where αj satisfy additional conditions depending on the semigroup. In the concrete case of [3] the conditions, giving (2.45), are (k 1) α =1+2πr , r Z, j =1,...,n. Sadiag − j j j ∈ In the framework of the above definitions, we can interpret the closed products (2.37)–(2.38) as the multiplications µ[3] of the ternary semigroups [3] (4, C)= N µ[3] . The corresponding querelements are given by Sstar1,2 star1,2 | 1 1 x 0 0 0 0 0 0 z 1 1 ¯ 1 0 0 z 0 ¯ 1 0 x 0 0 Nstar1 = Nstar− 1 = 1 , Nstar2 = Nstar− 2 = 1 , x,y,z,t =0. (2.46) 0 y 0 0 0 0 t 0 6 0 0 0 1 1 0 0 0 t y The ternary semigroups having querelements for each element (i.e. the additional operation ( ) defined by (2.46)) are the ternary groups [3] (4, C)= N µ[3], ( ) which are two (non-intersecting because N N = ∅) subgroups Gstar1,2 star1,2 | star1 ∩ star2 n [3] C o [3] C of the ternary general linear group GL (4, ). The ternary identities in star1,2 (4, ) are the following different continuous [3] [3] G sets Istar1,2 = Istar1,2 , where n o eiα1 0 0 0 iα2 [3] 0 0 e 0 2iα1 2iα4 i(α2+α3) R I = 3 , e = e = e =1, αj , (2.47) star1 0 eiα 0 0 ∈ 0 0 0 eiα4 0 0 0 eiα1 iα2 [3] 0 e 0 0 2iα2 2iα3 i(α1+α4) R I = 3 , e = e = e =1, αj . (2.48) star2 0 0 eiα 0 ∈ eiα4 0 0 0
In the particular case αj = 0, j = 1, 2, 3, 4, the ternary identities (2.47)–(2.48) coincide with the bisymmetric permutation matrices (2.28). Next we treat the closed set products (2.39)–(2.40) as the multiplications µ[5] of the 5-ary semigroups [5] (4, C) = Scirc1,2 N µ[5] . The querelements are circ1,2 | 1 1 0 0 yzt 0 0 yzt 0 0 1 1 ¯ 3 xzt 0 0 0 ¯ 3 0 0 0 xzt Ncirc1 = Ncirc− 1 = 1 , Ncirc2 = Ncirc− 2 = 1 , x,y,z,t =0. (2.49) 0 0 0 xyt xyt 0 0 0 6 0 1 0 0 0 0 1 0 xyz xyz and the corresponding 5-ary groups [5] (4, C) = N µ[5], ( ) which are two (non-intersecting because N Gcirc1,2 circ1,2 | circ1 ∩ [5] Ncirc2 = ∅) subgroups of the 5-ary general linear groupnGL (n, C). Weo have the following continuous sets of 5-ary identities 9
I[3] = I[3] in [5] (4, C) satisfying circ1,2 circ1,2 Gcirc1,2 n o 0 0 eiα1 0 iα2 [5] e 0 0 0 i(α1+α2+α3+α4) R I = 3 , e =1, αj , (2.50) circ1 0 0 0 eiα ∈ 0 eiα4 0 0 0 eiα1 0 0 iα2 [5] 0 0 0 e i(α1+α2+α3+α4) R I = 3 , e =1, αj . (2.51) circ2 eiα 0 0 0 ∈ 0 0 eiα4 0 In the case αj = 0, j = 1, 2, 3, 4, the 5-ary identities (2.50)–(2.51) coincide with the 90◦-symmetric permutation matrices (2.29). Thus, it follows from (2.46)–(2.51) that the 4-vertex star-like (2.35) and circle-like (2.36) matrices form subgroups of the k-ary general linear group GL[k] (4, C) with significantly different properties: they have different querelements and (sets of) [3] C [5] C polyadic identities, and even the arities of the subgroups star1,2 (4, ) and circ1,2 (4, ) do not coincide (2.37)–(2.40). If we take into account that 4-vertex star-like (2.35) and circle-likeG (2.36) matricesG are (binary) additive and distributive, then they form (with respect to the binary matrix addition (+) and the multiplications µ[3] and µ[5]) the (2, 3)-ring [3] (4, C) = Rstar1,2 [3] [5] C [5] Nstar1,2 +,µ and (2, 5)-ring circ1,2 (4, )= Nstar1,2 +,µ . Next we| consider the “interaction”R of the 4-vertex star-like (2.35)| and circle-like (2.36) matrix sets, i.e. their exotic module structure. For this, let us recall the ternary (polyadic) mo dule [44] and s-place action [45] definitions, which are suitable for our case. An abelian group is a ternary left (middle, right) -module (or a module over ), if there exists a ternary operation ( M , R ) which satisfies some compatibilityR conditions (associativity and R×R×M→Mdistributivity) which holdR×M×R→M in the matrix caseM×R×R→M under consideration (and where the module operation is the triple ordinary matrix product) [44]. A 5-ary left (right) module over is a 5-ary operation ( ) with analogous conditions (and where theM moduleR operation is the pentupleR×R×R×R×M matrix product) [45]. → M M×R×R×R×R → M First, we have the triple relations “inside” star and circle matrices
Nstar1 (Nstar2) Nstar1 = (Nstar2) , Ncirc1Ncirc2Ncirc1 = Ncirc1, (2.52)
Nstar1Nstar1 (Nstar2) = (Nstar2) , Ncirc1Ncirc1Ncirc2 = Ncirc1, (2.53)
(Nstar2) Nstar1Nstar1 = (Nstar2) , Ncirc2Ncirc1Ncirc1 = Ncirc1, (2.54)
Nstar2Nstar2 (Nstar1) = (Nstar1) , Ncirc2Ncirc2Ncirc1 = Ncirc2, (2.55)
Nstar2 (Nstar1) Nstar2 = (Nstar1) , Ncirc2Ncirc1Ncirc2 = Ncirc2, (2.56)
(Nstar1) Nstar2Nstar2 = (Nstar1) , Ncirc1Ncirc2Ncirc2 = Ncirc2. (2.57) We observe the following module structures on the left column above (elements of the corresponding module are in brackets, and we informally denote modules by their sets): 1) from (2.52)–(2.54), the set Nstar2 is a middle, right and left module over Nstar1; 2) from (2.55)–(2.57), the set Nstar1 is a middle, right and left module over Nstar2;
Nstar1Ncirc1Nstar1 = Ncirc2, Nstar1Ncirc2Nstar1 = Ncirc1, (2.58)
Nstar2Ncirc1Nstar2 = Ncirc2, Nstar2Ncirc2Nstar2 = Ncirc1, (2.59)
Nstar1Nstar1 (Ncirc1) = (Ncirc1) , (Ncirc1) Nstar1Nstar1 = (Ncirc1) , (2.60)
Nstar1Nstar1 (Ncirc2) = (Ncirc2) , (Ncirc2) Nstar1Nstar1 = (Ncirc2) , (2.61)
Nstar2Nstar2 (Ncirc1) = (Ncirc1) , (Ncirc1) Nstar2Nstar2 = (Ncirc1) , (2.62)
Nstar2Nstar2 (Ncirc2) = (Ncirc2) , (Ncirc2) Nstar2Nstar2 = (Ncirc2) , (2.63)
3) from (2.60)–(2.63), the sets Ncirc1,2 are a right and left module over Nstar1,2;
Ncirc1 (Nstar1) Ncirc1 = (Nstar1) , Ncirc1 (Nstar2) Ncirc1 = (Nstar2) , (2.64)
Ncirc2 (Nstar1) Ncirc2 = (Nstar1) , Ncirc2 (Nstar2) Ncirc2 = (Nstar2) , (2.65)
Ncirc1Ncirc1Nstar1 = Nstar2, Nstar1Ncirc1Ncirc1 = Nstar2, (2.66)
Ncirc1Ncirc1Nstar2 = Nstar1, Nstar2Ncirc1Ncirc1 = Nstar1, (2.67)
Ncirc2Ncirc2Nstar1 = Nstar2, Nstar1Ncirc2Ncirc2 = Nstar2, (2.68)
Ncirc2Ncirc2Nstar2 = Nstar1, Nstar2Ncirc2Ncirc2 = Nstar1, (2.69) 10
4) from (2.64)–(2.65), the sets Nstar1,2 are a middle ternary module over Ncirc1,2;
Ncirc1Ncirc1Ncirc1Ncirc1 (Nstar1) = (Nstar1) , Ncirc1Ncirc1Ncirc1Ncirc1 (Nstar2) = (Nstar2) , (2.70)
(Nstar1) Ncirc1Ncirc1Ncirc1Ncirc1 = (Nstar1) , (Nstar2) Ncirc1Ncirc1Ncirc1Ncirc1 = (Nstar2) , (2.71)
Ncirc2Ncirc2Ncirc2Ncirc2 (Nstar1) = (Nstar1) , Ncirc2Ncirc2Ncirc2Ncirc2 (Nstar2) = (Nstar2) , (2.72)
(Nstar1) Ncirc2Ncirc2Ncirc2Ncirc2 = (Nstar1) , (Nstar2) Ncirc2Ncirc2Ncirc2Ncirc2 = (Nstar2) , (2.73)
Ncirc1Ncirc1Ncirc1Ncirc1 (Ncirc2) = (Ncirc2) , (Ncirc2) Ncirc1Ncirc1Ncirc1Ncirc1 = (Ncirc2) , (2.74)
Ncirc2Ncirc2Ncirc2Ncirc2 (Ncirc1) = (Ncirc1) , (Ncirc1) Ncirc2Ncirc2Ncirc2Ncirc2 = (Ncirc1) . (2.75)
5) from (2.70)–(2.75), the sets Ncirc1,2 are right and left 5-ary modules over Ncirc2,1 and Nstar1,2. Note that the sum of 4-vertex star solutions of the Yang-Baxter equations (2.33) (with different parameters) gives the shape of 8-vertex matrices, and the same with the 4-vertex circle solutions (2.34). Let us introduce two kind of 8-vertex 4 4 matrices × over C: an 8-vertex star matrix Mstar and an 8-vertex circle matrix Mcirc as x 0 0 y 0 z s 0 M = , det M = (xw yv) (st uz) , tr M = x + z + u + w, (2.76) star 0 t u 0 star − − star v 0 0 w 0 x y 0 z 0 0 s M = , det M = (xw yv) (st uz) , tr M =0. (2.77) circ t 0 0 u circ − − circ 0 v w 0 If Mstar and Mcirc are invertible (the determinants in (2.76)–(2.77) are non-vanishing), then
w v w v xw yv 0 0 xw yv 0 xw yv xw yv 0 − u t − − u − − − t 1 0 st uz st uz 0 1 st uz 0 0 st uz M − = − ,M − = − , (2.78) star 0 s− −z 0 circ s− 0 0 −z st uz − st uz st uz − st uz y −0 0− x −0 y x 0− − xw yv xw yv − xw yv xw yv − − − − and therefore the parameter conditions for invertibility are the same in both Mstar and Mcirc xw yv =0, st uz =0. (2.79) − 6 − 6 The corresponding sets M = M and M = M are closed under the following multiplications star { star} circ { circ} MstarMstar = Mstar, (2.80)
MstarMcirc = Mcirc, McircMstar = Mcirc, (2.81)
McircMcirc = Mstar, (2.82) and in terms of sets we can write M = N N and M = N N , while N N = ∅ and star star1 ∪ star2 circ circ1 ∪ circ2 star1 ∩ star2 Ncirc1 Ncirc2 = ∅ (see (2.41)). Note that, if Mstar and Mcirc are treated as elements of an algebra, then (2.80)–(2.82) are reminiscent∩ of the Cartan decomposition (see, e.g., [46]), but we will consider them from a more general viewpoint, which will treat such structures as semigroups, ternary groups and modules. Thus the set M8vertex = Mstar Mcirc is closed, and because of the associativity of matrix multiplication, M8vertex forms a non-commutative semigroup∪ which we call a 8-vertex matrix semigroup (4, C), which contains the zero ma- S8vertex trix Z 8vertex (4, C) and is a subsemigroup of the (binary) general linear semigroup GLS (4, C). It follows from (2.80), ∈ S star C C that Mstar is its subsemigroup 8vertex (4, ). Moreover, the invertible elements of 8vertex (4, ) form a 8-vertex matrix group (4, C), because itsS identity is a unit 4 4 matrix I M , and so MS is a subgroup star (4, C) of G8vertex × 4 ∈ star star G8vertex 8vertex (4, C) and a subgroup of the (binary) general linear group GL (4, C). The structure of 8vertex (4, C) (2.80) is similar Gto that of block-diagonal and block-antidiagonal matrices (of the necessary sizes). So the 8-vertexS (binary) matrix semigroup S8vertex (4, C) in which the parameters satisfy (2.79) is a 8-vertex (binary) matrix group 8vertex (4, C), having a subgroup star (4, C)= M , I , where ( ) is an ordinary matrix product, and I is its identity.G G8vertex h star | · 4i · 4 The group structure of the circle matrices Mcirc (2.77) follows from
McircMcircMcirc = Mcirc, (2.83) which means that Mcirc is closed with respect to the product of three matrices (the product of two matrices from Mcirc is outside the set (2.82)). We define a ternary multiplication ν[3] as the ordinary triple product of matrices, then circ[3] (4, C)= S8vertex 11
[3] Mcirc ν is a ternary (3-nonderived) semigroup with the zero Z Mcirc which is a subsemigroup of the ternary (derived) | [3] ∈ general linear semigroup GLS (4, C). Instead of the inverse, for each invertible element Mcirc Mcirc Z we introduce the ¯ ∈ \ ¯ 1 unique querelement Mcirc [43] by (2.42), and since the ternary product is the triple ordinary product, we have Mcirc = Mcirc− from (2.43). Thus, if the conditions of invertibility (2.79) hold valid, then the ternary semigroup circ(3) (4, C) becomes the S8vertex ternary group circ(3) (4, C) = M ν[3], () which does not contain the ordinary (binary) identity, since I / M . G8vertex circ | 4 ∈ circ Nevertheless, the ternary group ofD circle matrices Ecirc[3] (4, C) has the following set I[3] = I[3] of left-right 6-vertex and G8vertex circ circ 8-vertex ternary identities (see (2.44)–(2.45)) n o
1 ab 1 ab 1 ad 0 a b 0 0 c c 0 0 c −c 0 ab − 1 cd − 1 ad [3] a 0 0 c 0 0 0 b b 0 0 −b Icirc = −1 , , − , (2.84) 0 0 0 c c 0 0 a c 0 0 a 0 0 c 0 0 b 0 0 0 b d 0 2 which (without additional conditions) depend upon the free parameters a,b,c,d C, b,c =0, and I[3] = I , I[3] M . ∈ 6 circ 4 circ ∈ circ In the binary sense, the matrices from (2.84) are mutually similar, but as ternary identities they are different. If we consider the second operation for matrices (as elements of a general matrix ring), the binary matrix addition (+), the star[2,2] structure of M8vertex = Mstar Mcirc becomes more exotic: the set Mstar is a (2, 2)-ring 8vertex = Mstar +, with ∪ star R h | circ·i[2,3] the binary addition (+) and binary multiplication ( ) from the semigroup 8vertex, while Mcirc is a (2, 3)-ring 8vertex = [3] · S [3] R Mcirc +,ν with the binary matrix addition (+), the ternary matrix multiplication ν and the zero Z. Moreover,| because of the distributivity and associativity of binary matrix multiplication, the relations (2.81) mean that the set circ Mcirc (being an abelian group under binary addition) can be treated as a left and right binary module 8vertex over the ring star(2,2) M 8vertex with an operation ( ): the moduleaction Mcirc Mstar = Mcirc, Mstar Mcirc = Mcirc (coinciding with the ordinary matrixR product (2.81)). The∗ left and right modules are∗ compatible, since the associativity∗ of ordinary matrix multiplication star(2,2) circ(2,3) gives the compatibility condition (McircMstar) Mcirc′ = Mcirc (MstarMcirc′ ), Mstar 8vertex , Mcirc,Mcirc′ 8vertex , ∈ R star(2∈,2) R and therefore Mcirc (as an abelian group under the binary addition (+) and the module action ( )) is a 8vertex -bimodule circ . The last relation (2.82) shows another interpretation of M as a formal “square root”∗ of M R(as sets). M8vertex circ star
F. Star 8-vertex and circle 8-vertex Yang-Baxter maps
Let us consider the star 8-vertex solutions c˜ to the Yang-Baxter equation (2.12), having the shape (2.76), in the most general setting, over C and for different ranks (i.e. including noninvertible ones). In components they are determined by
vy(u z)=0, y t2 wz x2 + xz =0, y(s(x z)+ t(u x))=0, y u(w x)+ x2 s2 =0, svy −tuz =0, tvy −suz =0− , vwy + xz(x z) −stz =0,− y w2 wz + xz −s2 =0, − uz(z− u)=0, suz − tvy =0, y(s(w u)+−t(z − w))=0, v s2 −wz x2 +−xz =0, (2.85) tuz −svy =0, stz −vxy + wz(z w)=0− , stu +− u2x ux2 vwy−=0,− v(s(z w)+ t(w u))=0, uz(u− z)=0, y t2−+ u(w x) −w2 =0, v(s(u x)+− t(x − z))=0, v s2 +−u(w x) −w2 =0, vy(z −u)=0, v u(w x)+− x2 − t2 =0, uw2 +−vxy stu − u2w =0, v w2 t2 −wz −+ xz =0. − − − − − − − Solutions from, e.g. [31, 35], etc., should satisfy this overdetermined system of 24 cubic equations for 8 variables. We search for the 8-vertex constant solutions to the Yang-Baxter equation over C without additional conditions, unitarity, etc. (which will be considered in the next sections). We also will need the matrix functions tr and det which are related to link invariants, as well as eigenvalues which help to find similar matrices and q-conjugated solutions to braid equations. Take into account that the Yang-Baxter maps are determined up to a general complex factor t C (2.14). For eigenvalues (which are ∈ determined up to the same factor t) we use the notation: eigenvalue [algebraic multiplicity]. We found the following 8-vertex solutions, classified by{ rank and number} of parameters. Rank =4 (invertible star Yang-Baxter maps) are 1)• quadratic in two parameters
2 xy 0 0 y trc ˜ =4xy, par=2 0 xy xy 0 4 4 c˜rank=4 (x, y)= ± , detc ˜ =4x y , x =0, y =0, (2.86) 0 xy xy 0 [2]6 6 [2] 2 ∓ eigenvalues: (1+ i) xy , (1 i) xy , x 0 0 xy { } { − } − 12
2) quadratic in three parameters
2 xy 0 0 y trc ˜ =2y (x + z) , par=3 0 zy xy 0 4 2 2 2 c˜rank=4,1 (x,y,z)= ± , detc ˜ = y z x , z = x, y =0, (2.87) 0 xy zy 0 − 6 ± 6 [2] 2 ± eigenvalues: y (x z) , y (x z) , y (x + z) , z 0 0 xy − − − { } 3) irrational in three parameters
xy 0 0 y2 2 2 0 x+z y y x +z 0 par=3 2 ± 2 trc ˜ =2y (x + z) , c˜rank=4 (x,y,z)= 2 2 , 1 4 4 (2.88) 0 y x +z qx+z y 0 det˜c = y (x z) , y =0,z = x, 2 2 16 − 6 6 2 ± (x+z) q0 0 yz 4 1 [2] 1 [2] eigenvalues: y x + z √2 x2 + z2 , y x + z + √2 x2 + z2 . 2 − 2 p p Note that only the first and the last cases are genuine 8-vertex Yang-Baxter maps, because the three-parameter matrices (2.87) are q-conjugated with the 4-vertex parameter-permutation solutions (2.33). Indeed,
xy 0 0 y2 y (x + z)0 0 0 0 zy xy 0 0 0 y (x z) 0 1 1 = (q K q) − q− K q− , (2.89) 0 xy zy 0 ⊗ 0 y (x z)0 0 ⊗ 2 − z 0 0 xy 0 0 0 y (x + z) y b q = ± z , (2.90) 1 b z p ∓ y ! q C y where b is a free parameter. If b = z two matrices q in (2.90) are similar, and we have the unique q-conjugation (2.89). Another solution∈ in (2.87) is q-conjugated to the second 4-vertex parameter-permutation solutions (2.33) such that
xy 0 0 y2 0 0 0 y (x z) − 0 zy xy 0 0 y (x + z)0 0 1 1 − = (q K q) q− K q− , (2.91) 0 xy zy 0 ⊗ 0 0 y (x + z) 0 ⊗ 2 − z 0 0 xy y (x z)0 0 0 − i y i y i y i y q = z z , z z , (2.92) 1± 1 − 1± 1 p± p ±p p where q’s are pairwise similar in (2.92), and therefore we have 2 different q-conjugations. Rank =2 (noninvertible star Yang-Baxter maps) are quadratic in parameters • xy 0 0 y2 par=2 0 xy xy 0 trc ˜ =4xy, c˜ (x, y)= ± , [2] [2] (2.93) rank=2 0 xy xy 0 eigenvalues: 2xy , 0 . 2 ± { } { } x 0 0 xy par=2 There are no star 8-vertex solutions of rank 3. The above two solutions for c˜rank=4 with different signs are q-conjugated (2.19) with the matrix q being one of the following
0 1 (2.94) q = i x 0 . ± y Further families of solutions can be obtained from (2.86)–(2.93) by applying the general q-conjugation (2.14). Particular cases of the star solutions are called also X-type operators [37] or magic matrices [18] connected with the Cartan decomposition of SU (4) [27, 28, 47, 48]. 13
The circle 8-vertex solutions c˜ to the Yang-Baxter equation (2.12) of the shape (2.77) are determined by the following system of 32 cubic equations for 8 unknowns over C
x(ty + z(u y) vx)=0, tx2 + y2(v z) wx2 =0,y( st + tx + wy xz)=0,su(x y) sxy + uxy =0, z(t(y x) −sz +−wx)=0, v sy + x2 − z −s2 + ux =0−,swy s2v + xy−(v z)=0,swx− s−2w + yz(u y)=0, st2 −t2x +−z2(y u)=0,su(v z)+ x−(xz tu)=0,su(w −v)+ xy(z t)=0− ,s(tu uw− + yz) ty2 −=0, s tv−+ z2 x v−2 + wz =0 ,svw− vwx + −z(xz wy)=0,− sw(w t)+−yz(z v)=0−,s(sz + u(v− w) vy)=0, t(tu vy +−z(y x))=0, tx(x s)+− u2v uvy =0− , xy(t w)+ u−2w uvx =0− ,t sy + u2 w ux− + y−2 =0, tz (s − x) sv2 +− tuv =0 ,tz(x − y) svw−+ uvw =0,u w−2 tz swz− + tyz =0,s2(t w)+− u2(v z)=0, tx(w− t)+− uv(z v)=0,tvx −t2y− uvw + vwy =0,tvy −t2u +−w(wy uz)=0,u (s(v− w) tu +−wx)=0 , twz −tv(w + z)+−vwz =0, v(s−(w −t) uw + vx)=0, sw 2− uv2 + v2y −w2x =0, w(sv +−u(z− v) wy)=0. − − − − − − − (2.95) We found the 8-vertex solutions, classified by rank and number of parameters. Rank =4 (invertible circle Yang-Baxter map) are quadratic in parameters • 0 xy yz 0 trc ˜ =0, z2 0 0 xy c˜par=3 (x,y,z)= , detc ˜ = y2z2 z2 x2 ,y =0, z =0, z = x, rank=4 xz 0 0 yz − 6 6 6 ± 2 eigenvalues: √ yz (x z) , √ yz (x z) , √yz (x + z) , √yz (x + z) . 0 z xz 0 − − − − − − (2.96) Rank =2 (noninvertible circle Yang-Baxter map) are linear in parameters • 0 y y 0 − − par=2 x 0 0 y [2] c˜ (x, y)= − , eigenvalues: 2√xy, 2√xy, 0 . (2.97) rank=2 x 0 0 y − { } − 0 x x 0 There are no circle 8-vertex solutions of rank 3. The corresponding families of solutions can be derived from the above by using the q-conjugation (2.14). A particular case of the 8-vertex circle solution (2.96) was considered in [49].
G. Triangle invertible 9- and 10-vertex solutions
There are some higher vertex solutions to the Yang-Baxter equations which are not in the above star/circle classification. They are determined by the following system of 15 cubic equations for 9 unknowns over C
y( py x(u + w y)+ v(y + z)) + s(v x)(v + x)=0, x( ty + vz + x(y z))=0, − − − − − − sx(t v)+ ty(w z)+ vz(y u)=0, z(pz t(y + z)+ x(u + w z)) + s x2 t2 =0, − − − − − − ps( u + w y + z)+ s( t(u + z)+ x(u w + y z)+ v(w + y)) + uwy uwz uyz + wyz =0, − − − − − − − t(y(p t)+ u(x v))=0, t(pz t(u + z)+ ux)=0, − − − p2s + pu( u + y + z) t(st + u(u + w)) + u2x =0, t(z(p v) tw + wx)=0, − − − − ps(t v)+ tw(y u)+ uv(w z)=0, v( py + v(w + y) wx)=0, − − − − − v(z(v p)+ tw wx)=0, v(y(t p)+ u(v x))=0, − − − − p2( s)+ pw(w y z)+ sv2 + w(v(u + w) wx)=0, p(p(w u) tw + uv)=0, (2.98) − − − − − − We found the following 9-vertex Yang-Baxter maps
xyz s xy y z x y y z − zx 9 vert,1 0 0 x y 0 0 x y 0 0 x y c˜ − = , , − , (2.99) rank=4 0 x 0 z 0 x −0 −y 0 x 0 zx − − y 0 0 0 x 00 0 x 00 0 x [3] trc ˜ =2x, detc ˜ = x4, x =0, eigenvalues: x , x. (2.100) − 6 { } − 14
The third matrix in (2.99) is conjugated with the 4-vertex parameter-permutation solutions (2.33) of the form (which has the same the same eigenvalues (2.100))
x 0 0 0 4 vert 0 0 x 0 c˜ − (x)= (2.101) rank=4 0 x 0 0 0 0 0 x by the conjugated matrix
y y 1 2x 2x 0 0− 1 0 z U 9to4 = − y . (2.102) 00 1 0 00 0 1 The matrix (2.102) cannot be presented as the Kronecker product q K q (2.16), and so the third matrix in (2.99) and (2.101) are different solutions of the Yang-Baxter equation (2.12). Despite⊗ the first two matrices in (2.99) have the same eigenvalues (2.100), they are not similar, because they have different from (2.101) middle Jordan blocks. Then we have another 3-parameter solutions with fractions
2 xyy z 2xz y 2xz trc ˜ =2x y−2 , 0 0 x y 2 9 vert,2 − − y 4 4xz 3y c˜ − (x,y,z)= 2xz , detc ˜ = x 3 y2 , x =0, y =0, z = 4x , (2.103) rank=4 0 x 0 y y − 6 6 6 − − [2] 4xz 4xz eigenvalues: x , x, x 2 3 , 00 0 x 2 3 y y − { } − − and
xz x y y z trc ˜ =2x 1+2 2 − 2zx y 0 0 x + y 2 9 vert,3 − y 4 4zx y c˜rank− =4 (x,y,z)= 2zx , detc ˜ =3x y2 +1 , x =0, y =0, z = 4x (2.104) 0 3x 0 y y 6 6 6 2 − 4zx √ √ 4zx 00 0 2 + x eigenvalues: x, i 3x, i 3x, x 1+ y2 y − The 4-parameter 9-vertex solution is
xyz s 2sx 2sx yz 9 vert,par=4 0 0 x y trc ˜ =2x −2 z 4 z c˜rank− =4 (x,y,z,s)= 2xy − − 2sx , x (2y z)(z(2y+z) 4sx) z 0 x z 0 z z detc ˜ = − 3 − , x =0,y = ,z =0, − x(4sx−z(2y+z)) z 6 6 2 6 0 0 0 − 2 z (2.105) 2y 2y x(4sx z(2y + z)) eigenvalues: (2.106) x, x 1, x 1, − 2 . r z − − r z − z We also found 5-parameter, 9-vertex solution of the form
xyz s s(t x) 9 vert,par=5 0 0 t −z + y c˜ − (x,y,z,s,t)= y(t x) s(t x) , (2.107) rank=4 0 − + x 0 − + z z 2 z s(t x) +tz(y+z) xyz 0 0 0 − 2 − z st2 + sx2 + tz2 + xz2 2stx + tyz xyz trc ˜ = − − , (2.108) z2 xt (x (y z) ty) s (t x)2 + tz (y + z) xyz detc ˜ = − − − − , x =0, z =0, t =0, (2.109) z3 6 6 6 t t st2 2stx + tz2 + ytz + sx2 yxz eigenvalues: (2.110) x, (ty xy + xz), (ty xy + xz), − 2 − . rz − −rz − z 15
Finally, we found the following 3-parameter 10-vertex solution
2 y xy y x trc ˜ =2x, 10 vert 0 0 x y detc ˜ = x x3 + zy2 , x =0, c˜rank− =4 (x,y,z)= − − , (2.111) 0 x 0 y − 2 6 2 eigenvalues: x [2] , x2 + zy , x2 + zy . z −0 0 −x x x { } − q q This solution is conjugated with the 4-vertex parameter-permutation solutions (2.33) of the form (which has the same the same eigenvalues as (2.111))
x 0 0 0 2 y z 4 vert 0 0 x + 2 0 c˜ − (x,y,z)= x (2.112) rank=4 0 x 0 0 00 0 x by the conjugated matrix
0 x x 0 z 2 2z x −x y 10to4 1 yz yz x 2 2 U = − − x x − . (2.113) 1 yz yz 0 − 0 0 1 1 Because the matrix (2.113) cannot be presented as the Kronecker product q K q (2.16), therefore (2.111) and (2.112) are different solutions of the Yang-Baxter equation (2.12). ⊗ Further families of the higher vertex solutions to the constant Yang-Baxter equation (2.12) can be obtained from the above ones by using the q-conjugation (2.14).
III. POLYADIC BRAID OPERATORS AND HIGHER BRAID EQUATIONS
The polyadic version of the braid equation (2.1) was introduced in [21]. Here we define higher analog of the Yang-Baxter operator and develop its connection with higher braid groups and quantum computations. Let us consider a vector space V over a field K.A polyadic (n-ary) braid operator CVn is defined as the mapping [21]
n n
C n : V ... V V ... V. (3.1) V ⊗ ⊗ → ⊗ ⊗ The polyadic analog of the braid equation (2.1) wasz introduc}| ed{ inz [21] using}| the{ associative quiver technique [45]. Let us introduce n operators
2n 1 2n 1 − − A : V ... V V ... V, (3.2) p ⊗ ⊗ → ⊗ ⊗ (p 1) (n p) A =z id⊗ }|− {C nz id}|⊗ − {, p =1, . . . , n, (3.3) p V ⊗ V ⊗ V n i.e. p is a place of C n instead of one id in id⊗ . A system of (n 1) polyadic (n-ary) braid equations is defined by V V V −
A1 A2 A3 A4 ... An 2 An 1 An A1 (3.4) ◦ ◦ ◦ ◦ ◦ − ◦ − ◦ ◦ = A2 A3 A4 A5 ... An 1 An A1 A2 (3.5) ◦ ◦ ◦ ◦ ◦ − ◦ ◦ ◦ . .
= An A1 A2 A3 ... An 3 An 2 An 1 An. (3.6) ◦ ◦ ◦ ◦ ◦ − ◦ − ◦ − ◦
Example 1. In the lowest non-binary case n =3, we have the ternary braid operator CV3 : V V V V V V and two 5 ⊗ ⊗ → ⊗ ⊗ ternary braid equations on V⊗
(C 3 id id ) (id C 3 id ) (id id C 3 ) (C 3 id id ) V ⊗ V ⊗ V ◦ V ⊗ V ⊗ V ◦ V ⊗ V ⊗ V ◦ V ⊗ V ⊗ V = (id C 3 id ) (id id C 3 ) (C 3 id id ) (id C 3 id ) V ⊗ V ⊗ V ◦ V ⊗ V ⊗ V ◦ V ⊗ V ⊗ V ◦ V ⊗ V ⊗ V = (id id C 3 ) (C 3 id id ) (id C 3 id ) (id id C 3 ) . (3.7) V ⊗ V ⊗ V ◦ V ⊗ V ⊗ V ◦ V ⊗ V ⊗ V ◦ V ⊗ V ⊗ V 16
Note that the higher braid equations presented above differ from the generalized Yang-Baxter equations of [23, 24, 50]. The higher braid operators (3.1) satisfying the higher braid equations (3.4)–(3.6) can represent the higher braid group [22] using (2.6) and (3.3). By analogy with (2.6) we introduce m operators by
m+n 2 m+n 2 − − (m+n 2) B (m): V ... V V ... V, B (m) = (id )⊗ − , (3.8) i ⊗ ⊗ → ⊗ ⊗ 0 V (i 1) (m i 1) B (m) =z id⊗ }|− {C nz id⊗}| − −{ , i =1,...,m 1. (3.9) i V ⊗ V ⊗ V − [n] [n+1] The representation πm of the higher braid group m (of (n + 1)-degree in the notation of [22]) (having m 1 generators B − σi and identity e) is given by [n] [n+1] (m+n 2) π : End V⊗ − , (3.10) m Bm −→ π[n] (σ )=B (m) , i =1,...,m 1. (3.11) m i i − [n+1] In this way, the generators σi of the higher braid group m satisfy the relations n higher braid relations B • n+1
σiσi+1 ... σi+n 2σi+n 1σi (3.12) − − = σi+1σi+2 ... σi+n 1σiσi+1 (3.13) z }| − { . .
= σi+n 1σiσi+1σi+2 ... σiσi+1σi+n 1, (3.14) − − i =1,...,m n, (3.15) − n-ary far commutativity • n σ σ σ σ σ i1 i2 ... in−2 in−1 in (3.16) . z. }| { σ σ σ σ σ = τ(i1) τ(i2) ... τ(in−2) τ(in−1) τ(in), (3.17) if all i i n, p,s =1, . . . , n, (3.18) | p − s|≥ where τ is an element of the permutation symmetry group τ Sn. The relations (3.12)–(3.17) coincide with those from [22], obtained by another method, that is via the polyadic-binary correspondence.∈ [4] σ σ σ In the case m = 4 and n = 3 the higher braid group 4 is represented by (3.7) and generated by 3 generators 1, 2, 3, which satisfy 2 braid relations only (without far commutatiB vity)
σ1σ2σ3σ1 = σ2σ3σ1σ2 = σ3σ1σ2σ3. (3.19) According to (3.16)–(3.17), the far commutativity relations appear when the number of elements of the higher braid groups satisfy m m = n (n 1)+2, (3.20) ≥ min − such that all conditions (3.18) should hold. Thus, to have the far commutativity relations in the ordinary (binary) braid group (2.5) we need 3 generators and , while for n =3 we need at least 7 generators σ and [4] (see Example 7.12 in [22]). B4 i B8 In the concrete realization of V as a d-dimensional euclidean vector space Vd over the complex numbers C and basis ei , n n { } i =1,...,d, the polyadic (n-ary) braid operator CVn becomes a matrix Cdn of size d d which satisfies n 1 higher braid equations (3.4)–(3.6) in matrix form. In the components, the matrix braid operator is × −
d ′ ′ ′ j1j2...jn n ′ ′ ′ (3.21) Cd (ei1 ei2 ... ein )= ci1i2...in ej1 ej2 ... ejn . ◦ ⊗ ⊗ ⊗ ′ ′ ′ · ⊗ ⊗ ⊗ j1,j2X...jn=1 2n 4n 2 THUS we have d entries (unknowns) in Cdn satisfying (n 1) d − equations (3.4)–(3.6) in components of polynomial power n+1. In the minimal non-binary case n =3, we have 2d10−equations of power 4 for d6 unknowns, e.g. even for d =2 we have 2048 for 64 components, and for d = 3 there are 118 098 equations for 729 components. Thus solving the matrix higher braid equations directly is cumbersome, and only particular cases are possible to investigate, for instance by using permutation matrices (2.28), or the star and circle matrices (2.76)–(2.77). 17
IV. SOLUTIONS TO THE TERNARY BRAID EQUATIONS
Here we consider some special solutions to the minimal ternary version (n = 3) of the polyadic braid equation (3.4)–(3.6), the ternary braid equation (3.7).
A. Constant matrix solutions
Let us consider the following two-dimensional vector space V Vd=2 (which is important for quantum computations) and the component matrix realization (3.21) of the ternary braiding operator≡ C : V V V V V V as 8 ⊗ ⊗ → ⊗ ⊗
2 ′ ′ ′ j1j2j3 ′ ′ ′ C8 (ei1 ei2 ei3 )= ci1i2i3 ej1 ej2 ej3 , i1,2,3, j1′ ,2,3 =1, 2. (4.1) ◦ ⊗ ⊗ ′ ′ ′ · ⊗ ⊗ j1,jX2,j3=1
We now turn (4.1) to the standard matrix form (just to fix notations) by introducing the 8-dimensional vector space V˜8 = ˜ V V V with the natural basis e˜k˜ = e1 e1 e1,e1 e1 e2,...,e2 e2 e2 , where k = 1,..., 8 is a cumulative ⊗ ⊗ { ⊗ ⊗ ⊗ ⊗ ⊗ ⊗ } 8 index. The linear operator C˜ : V˜ V˜ corresponding to (4.1) is given by the 8 8 matrix c˜ ˜ as C˜ e˜ = c˜ ˜ e˜˜. The 8 8 → 8 × ˜ıj 8 ◦ ˜ı ˜j=1 ˜ıj · j operators (3.2)–(3.3) become three 32 32 matrices A˜ as × 1,2,3 P A˜ =˜c I I , A˜ = I c˜ I , A˜ = I I c,˜ (4.2) 1 ⊗K 2 ⊗K 2 2 2 ⊗K ⊗K 2 3 2 ⊗K 2 ⊗K where K is the Kronecker product of matrices and I2 is the 2 2 identity matrix. In this notation the operator ternary braid equations⊗ (3.7) become the matrix equations (cf. (3.4)–(3.6)) with×n =3)
A˜1A˜2A˜3A˜1 = A˜2A˜3A˜1A˜2 = A˜3A˜1A˜2A˜3, (4.3) which we call the total matrix ternary braid equations. Some weaker versions of ternary braiding are described by the partial braid equations
partial 12-braid equation A˜1A˜2A˜3A˜1 = A˜2A˜3A˜1A˜2, (4.4)
partial 13-braid equation A˜1A˜2A˜3A˜1 = A˜3A˜1A˜2A˜3, (4.5)
partial 23-braid equation A˜2A˜3A˜1A˜2 = A˜3A˜1A˜2A˜3, (4.6) where, obviously, two of them are independent. It follows from (3.4)–(3.6) that the weaker versions of braiding are possible for n 3, only, so for higher than binary braiding (the Yang-Baxter equation (2.8)). ≥ Thus, comparing (4.3) and (3.19) we conclude that (for each invertible matrix c˜ in (4.2) satisfying (4.3)) the isomorphism [4] σ ˜ [4] C π˜4 : i Ai, i =1, 2, 3 gives a representation of the braid group 4 by 32 32 matrices over . Now we7→ can generate families of solutions corresponding to (4.2)–(4.3)B in the× following way. Consider an invertible operator Q : V V in the two-dimensional vector space V Vd=2. In the basis e1,e2 its 2 2 matrix q is given by Q ei = 2 → ≡ { } × ◦ q e . In the natural 8-dimensional basis e˜˜ the tensor product of operators Q Q Q is presented by the Kronecker j=1 ij · j k ⊗ ⊗ product of matrices q˜8 = q K q K q. Let the 8 8 matrix c˜ be a fixed solution to the ternary braid matrix equations (4.3). ThenP the family of solutions⊗c˜(q) corresponding⊗ to× the invertible 2 2 matrix q is the conjugation of c˜ by q˜ so that × 8 1 1 1 1 c˜(q)=˜q c˜q˜− = (q q q)˜c q− q− q− . (4.7) 8 8 ⊗K ⊗K ⊗K ⊗K This also follows directly from the conjugation of the braid equations (4.3)–(4.6) by q K q K q K q K q and (4.2). If we include the obvious invariance of the braid equations with the respect of an overall factor⊗t C⊗, the⊗ general⊗ family of solutions becomes (cf. the Yang-Baxter equation [35]) ∈
1 1 1 1 c˜(q,t)= tq˜ c˜q˜− = t (q q q)˜c q− q− q− . (4.8) 8 8 ⊗K ⊗K ⊗K ⊗K Let
a b q = GL (2, C) , (4.9) c d ∈ 18 and then the manifest form of q˜8 is
a3 a2b a2b ab2 a2b ab2 ab2 b3 a2c a2d abc abd abc abd b2c b2d a2c abc a2d abd abc b2c abd b2d 2 2 2 2 ac acd acd ad bc bcd bcd bd q˜8 = 2 2 2 2 . (4.10) a c abc abc b c a d abd abd b d 2 2 2 2 ac acd bc bcd acd ad bcd bd 2 2 2 2 ac bc acd bcd acd bcd ad bd c3 c2d c2d cd2 c2d cd2 cd2 d3 It is important that not every conjugation matrix has this very special form (4.10), and that therefore, in general, conjugated ⋆ ⋆ matrices are different solutions of the ternary braid equations (4.3). The matrix q˜8 q˜8 ( being the Hermitian conjugation) is diagonal (this case is important for further classification similar to the binary one [31]), when the conditions
ab∗ + cd∗ =0 (4.11) hold, and so the matrix q has the special form (depending of 3 complex parameters, for d =0) 6 a b ∗ q = b . (4.12) a ∗ d − d We can present the families (4.7) for different ranks, because the conjugation by an invertible matrix does not change rank. To avoid demanding (4.11), due to the cumbersome calculations involved, we restrict ourselves to a triangle matrix for q (4.9). In general, there are 8 8 = 64 unknowns (elements of the matrix c˜), and each partial braid equation (4.4)–(4.6) gives 32 32 = 1024 conditions× (of power 4) for the elements of c˜, while the total braid equations (4.3) give twice as many conditions 1024× 2 = 2048 (cf. the binary case: 64 cubic equations for 16 unknowns (2.8)). This means that even in the ternary case the higher× braid system of equations is hugely overdetermined, and finding even the simplest solutions is a non-trivial task.
B. Permutation and parameter-permutation 8-vertex solutions
First we consider the case when c˜ is a binary (or logical) matrix consisting of 0, 1 only, and, moreover, it is a permutation { } matrix (see Subsection IID). In the latter case c˜ can be considered as a matrix over the field F2 (Galois field GF (2)). In total, there are 8! = 40320 permutation matrices of the size 8 8. All of them are invertible of full rank 8, because they are obtained from the identity matrix by permutation of rows and columns.× We have found the following four invertible 8-vertex permutation matrix solutions to the ternary braid equations (4.3)
10000000 00000001 00000010 01000000 00100000 00000100 trc ˜ =4, bisymm1 00001000 bisymm2 00010000 detc ˜ =1, c˜rank=8 = , c˜rank=8 = , (4.13) 00010000 00001000 [4] [4] eigenvalues: 1 , 1 , 00000100 00100000 { } {− } 01000000 00000010 00000001 10000000 10000000 00000100 00001000 01000000 00000001 00100000 trc ˜ =4, symm1 00010000 symm2 00000010 detc ˜ =1, c˜rank=8 = , c˜rank=8 = , (4.14) 01000000 00001000 [4] [4] eigenvalues: 1 , 1 . 00000100 10000000 { } {− } 00000010 00010000 00100000 00000001 The first two solutions (4.13) are given by bisymmetric permutation matrices (see (2.31)), and we call them 8-vertex bisymm1 and bisymm2 respectively. The second two solutions (4.14) are symmetric matrices only (we call them 8-vertex symm1 and symm2), but one matrix is a reflection of the other with respect to the minor diagonal (making them mutually persymmetric). No 90◦-symmetric (see (2.32)) solution for the ternary braid equations (4.3) was found. The bisymmetric and symmetric matrices 19 have the same eigenvalues, and are therefore pairwise conjugate, but not q-conjugate, because the conjugation matrices do not have the form (4.10). Thus they are 4 different permutation solutions to the ternary braid equations (4.3). Note that the bisymm1 solution (4.13) coincides with the three-qubit swap operator introduced in [18]. 2 All the permutation solutions are reflections (or involutions) c˜ = I8 having detc ˜ = +1, eigenvalues 1, 1 , and are semi- magic squares (the sums in rows and columns are 1, but not the sums in both diagonals). The 8-vertex{ permutation− } matrix solutions do not form a binary or ternary group, because they are not closed with respect to multiplication. By analogy with (2.33)–(2.34), we obtain the 8-vertex parameter-permutation solutions from (4.13)–(4.14) by replacing units with parameters and then solving the ternary braid equations (4.3). Each type of the permutation solutions bisymm1, 2 and symm1, 2 from (4.13)–(4.14) will give a corresponding series of parameter-permutation solutions over C. The ternary braid maps are determined up to a general complex factor (see (2.14) for the Yang-Baxter maps and (4.8)), and therefore we can present all the parameter-permutation solutions in polynomial form. The bisymm1 series consists of 2 two-parameter matrices with and 2 two-parameter matrices • xy 000 0000 0000 00 y2 0 0 0 xy 0 0000± 2 trc ˜ =4xy, bisymm1,1 0 0 0 0 x 0 0 0 detc ˜ = x8y8, x,y =0, c˜rank=8 (x, y)= 2 ± , (4.15) 0 0 0 y 0 0 0 0 [6] 6 [2] ± eigenvalues: xy , xy , 0000 0 xy 0 0 { } {− } 2 0 x 00 0000 0000± 000 xy
xy 000 0000 0000 00 y2 0 0 0 xy 0 0000± 2 trc ˜ =4xy, bisymm1,2 0 0 0 0 x 0 0 0 detc ˜ = x8y8, x,y =0, c˜rank=8 (x, y)= 2 ± , (4.16) 0 0 0 y 0 0 0 0 [4] [2]6 [2] ∓ eigenvalues: xy , ixy , ixy . 0000 0 xy 0 0 { } { } {− } 2 0 x 00 0000 0000∓ 000 xy The bisymm2 series consists of 4 two-parameter matrices • 0000 000 x6 0 x3y3 00 0000 00± 0 0 0 x4y2 0 0 3 3 3 3 bisymm2,1 0 0 0 x y 0 0 00 trc ˜ = 4x y , c˜rank=8 (x, y)= ± 3 3 , bisymm2 ± 24 24 00 0 0 x y 0 0 0 detc ˜rank=8 (x, y)= x y , x,y =0, 2 4 ± 6 0 0 x y 0 0 0 00 3 3 00 0 0 00 x y 0 y6 000 0000± (4.17) [2] [2] [4] eigenvalues: x3y3 , x3y3 , x3y3 , − ± 00 0 0 000 x6 0 x3y3 0 0 0000 00± 0 0 0 x4y2 0 0 3 3 3 3 bisymm2,2 0 0 0 x y 0 0 00 trc ˜ = 4x y c˜rank=8 (x, y)= ± 3 3 , bisymm2 ± 24 24 00 0 0 x y 0 0 0 detc ˜rank=8 (x, y)= x y ,x,y =0, 2 4 ± 6 0 0 x y 0 0 0 00 − 3 3 00 0 0 00 x y 0 y6 0 0 0 0000± − (4.18) [2] [2] [4] eigenvalues: ix3y3 , ix3y3 , x3y3 . − ± 20
The symm1 series consists of 4 two-parameter matrices •
xy 0 00 0 000 0 0 00 xy 0 0 0 ± 2 0 000 0 00 y trc ˜ =4xy, symm1,1 0 0 0 xy 0 000 detc ˜ = x8y8, x,y =0, c˜rank=8 (x, y)= , (4.19) 0 xy 00 0 000 [6] 6 [2] ± eigenvalues: xy , xy , 0 0 00 0 xy 0 0 { } {− } 0 000 0 0 xy 0 0 0 x2 0 0 000
xy 0 000000 00 00 xy 0 0 0 ± 2 00 00000 y trc ˜ =4xy, symm1,2 0 0 0 xy 0 000 detc ˜ = x8y8, x,y =0, c˜rank=8 (x, y)= , (4.20) 0 xy 0 0 0 000 [6] 6 [2] ∓ eigenvalues: xy , xy , 00 000 xy 0 0 { } {− } 00 0000 xy 0 0 0 x2 0 0 000 −
The symm2 series consists of 4 two-parameter matrices •
000 0 0 y2 0 0 0 xy 0 0 000 0 0 0 xy 0 00 0 0 trc ˜ =4xy, symm2,1 000 0 00 xy 0 detc ˜ = x8y8, x,y =0, c˜rank=8 (x, y)= ± , (4.21) 000 0 xy 0 0 0 [4] [2]6 [2] 2 eigenvalues: xy , ixy , ixy . x 00 0 000 0 { } { } {− } 0 0 0 xy 00 0 0 000± 0 00 0 xy
0 00 0 0 y2 0 0 0 xy 0 0 000 0 0 0 xy 0 00 0 0 trc ˜ =4xy, symm2,2 0 00 0 00 xy 0 detc ˜ = x8y8, x,y =0, c˜rank=8 (x, y)= ± , (4.22) 0 00 0 xy 0 0 0 [4] [2]6 [2] 2 eigenvalues: xy , ixy , ixy . x 00 0 000 0 { } { } {− } −0 0 0 xy 00 0 0 0 00∓ 0 000 xy
The above matrices with the same eigenvalues are similar, but their conjugation matrices do not have the form of the triple Kronecker product (4.10), and therefore all of them together are 16 different two-parameter invertible solutions to the ternary braid equations (4.3). Further families of solutions can be obtained using ternary q-conjugation (4.8).
C. Group structure of the star and circle 8-vertex matrices
Here we investigate the group structure of 8 8 matrices by analogy with the star-like (2.35) and circle-like (2.36) 4 4 matrices which are connected with our 8-vertex constant× solutions (4.15)–(4.22) to the ternary braid equations (4.3). × 21
Let us introduce the star-like 8 8 matrices (cf. (2.35)) which correspond to the bisymm series (4.15)–(4.18) × x 0000000 0000000 y 000000 y 0 0 x 000000 0 0 z 00000 00000 s 0 0 0000 s 00 0 0 0 0 z 0000 Nstar′ 1 = , Nstar′ 2 = , (4.23) 0 0 0 t 000 0 0000 u 0 0 0 00000 u 0 0 0 0 t 00000 0 v 000000 000000 w 0 0000000 w v 0000000 tr N ′ = x + z + u + w, det N ′ = stuvwxyz, s,t,u,v,w,x,y,z =0, 6 eigenvalues: x, z, u, w, √yv, √yv, √st, √st, − − and the circle-like 8 8 matrices (cf. (2.36)) which correspond to the symm series (4.19)–(4.22) × x 0000000 00000 y 0 0 0000 y 0 00 0 x 000000 0000000 z 0 0 s 0 0000 00 0 s 0000 000000 z 0 Ncirc′ 1 = , Ncirc′ 2 = , (4.24) 0 t 000000 000 0 u 0 0 0 00000 u 0 0 t 0000000 000000 v 0 0 0 0 w 0000 0 0 w 00000 0000000 v tr N = x + s + u + v, detN = stuvwxyz, s,t,u,v,w,x,y,z =0 , ′ ′ (4.25) eigenvalues: x, s, u, v, √ty, √ty, √wz, √wz. 6 − −
Denote the corresponding sets by Nstar′ 1,2 = Nstar′ 1,2 and Ncirc′ 1,2 = Ncirc′ 1,2 , then we have for them (which differs from 4 4 matrix sets (2.41)) ×
M′ = N′ N′ N′ N′ , N′ N′ N′ N′ = D, (4.26) full star1 ∪ star2 ∪ circ1 ∪ circ2 star1 ∩ star2 ∩ circ1 ∩ circ2 where D is the set of diagonal 8 8 matrices. Again, as for 4 4 star-like and circle-like matrices, there are no closed binary multiplications among the sets of×8-vertex matrices (4.23)–(4.24).× Nevertheless, we have the following triple set products
Nstar′ 1Nstar′ 1Nstar′ 1 = Nstar′ 1, (4.27)
Nstar′ 2Nstar′ 2Nstar′ 2 = Nstar′ 2, (4.28)
Ncirc′ 1Ncirc′ 1Ncirc′ 1 = Ncirc′ 1, (4.29)
Ncirc′ 2Ncirc′ 2Ncirc′ 2 = Ncirc′ 2, (4.30) which should be compared with the analogous 4 4 matrices (2.39)–(2.40): note that now we do not have pentuple products. × Using the definitions (2.42)–(2.45), we interpret the closed products (4.27)–(4.28) and (4.29)–(4.30) as the multiplications µ[3] [3] C [3] [3] C (being the ordinary triple matrix product) of the ternary semigroups star1,2 (8, ) = Nstar′ 1,2 µ and circ1,2 (8, ) = [3] S | S N′ µ , respectively. The corresponding querelements (2.42) are given by circ1,2 | 1 1 x 0000000 0000000 v 1 1 000000 v 0 0 x 000000 1 1 0 0 z 00000 00000 t 0 0 1 1 ¯ 1 0000 t 0 0 0 ¯ 1 0 0 0 z 000 0 Nstar′ 1 = Nstar′− 1 = 1 , Nstar′ 2 = Nstar′− 2 = 1 ,s,t,u,v,w,x,y,z =0, 0 0 0 s 000 0 0000 u 0 0 0 6 1 1 00000 u 0 0 0 0 s 00000 1 1 0 y 000000 000000 w 0 1 0000000 1 0000000 w y (4.31) 22 and
1 1 x 0000000 00000 t 0 0 1 1 0000 t 0 0 0 0 x 000000 1 1 0000000 w 0 0 s 00000 1 1 ¯ 1 0 0 0 s 000 0 ¯ 1 000000 w 0 Ncirc′ 1 = Ncirc′− 1 = 1 , Ncirc′ 2 = Ncirc′− 2 = 1 ,s,t,u,v,w,x,y,z =0. 0 y 000000 0000 u 0 0 0 6 1 00000 1 0 0 0000000 u y 000000 1 0 0 0 0 1 000 0 v z 0 0 1 00000 0000000 1 z v (4.32) [3] [3] [3] [3] The ternary semigroups (8, C)= N′ µ and (8, C)= N′ µ in which every element has Sstar1,2 star1,2 | Scirc1,2 circ1,2 | [3] [3] [3] its querelement given by (4.31)–(4.32) become the ternary groups (8, C)= N′ µ , ( ) and (8, C)= Gstar1,2 star1,2 | Gcirc1,2 [3] n o N′ µ , ( ) , which are four different (3-nonderived) ternary subgroups of the derived ternary general linear group circ1,2 | [3] [3] [3] [3] GLn (8, C). The ternaryo identities in (8, C) and (8, C) are the following different continuous sets I′ = Gstar1,2 Gcirc1,2 star1,2 [3] [3] [3] Istar′ 1,2 and Icirc′ 1,2 = Icirc′ 1,2 , where n o n o eiα1 0000000 0000000 eiα2 000000 eiα2 0 0 eiα1 000000 0 0 eiα3 0 0 0 0 0 0 0 0 0 0 eiα4 0 0 iα4 iα3 [3] 0 0 0 0 e 0 0 0 [3] 0 0 0 e 0 0 0 0 ′ ′ Istar1 = iα5 , Istar2 = iα6 , 0 0 0 e 0 0 0 0 0 0 0 0 e 0 0 0 iα6 iα5 0 0 0 0 0 e 0 0 0 0 e 0 0 0 0 0 iα7 iα8 0 e 000000 000000 e 0 iα8 iα7 0000000 e e 0000000 e2iα1 = e2iα3 = e2iα6 = e2iα8 = ei(α2+α7) = ei(α4+α5) =1, α ,...,α R, (4.33) 1 8 ∈ and eiα1 0000000 0 0 0 0 0 eiα2 0 0 0 0 0 0 eiα2 0 0 0 0 eiα1 000000 0000000 eiα3 0 0 eiα4 0 0 0 0 0 iα4 iα3 [3] 0 0 0 e 0 0 0 0 [3] 000000 e 0 ′ ′ Icirc1 = iα5 , Icirc2 = iα6 , 0 e 000000 0 0 0 0 e 0 0 0 iα6 iα5 0 0 0 0 0 e 0 0 e 0000000 iα7 iα8 000000 e 0 0 0 0 e 0 0 0 0 iα8 iα7 0 0 e 0 0 0 0 0 0000000 e e2iα1 = e2iα4 = e2iα6 = e2iα7 = ei(α3+α8) = ei(α2+α5) =1, α ,...,α R, (4.34) 1 8 ∈ [3] 2 such that all the identities are the 8 8 matrix reflections I′ = I8 (see (2.45)). If αj =0, j =1,..., 8, the ternary identities (4.33)–(4.34) coincide with the 8 ×8 permutation matrices (4.13)–(4.14), which are solutions to the ternary braid equations (4.3). The module structure of the 8-vertex× star-like (4.23) and circle-like (4.24) 8 8 matrix sets differs from the 4 4 matrix sets (2.52)–(2.75). Firstly, because of the absence of pentuple matrix products (2.70)–(2.75),× and secondly through some× differences in the ternary closed products of sets. We have the following triple relations between star and circle matrices separately (the sets corresponding to modules are in brackets, and we informally denote modules by their sets)
Nstar′ 1 (Nstar′ 2) Nstar′ 1 = (Nstar′ 2) , Ncirc′ 1 (Ncirc′ 2) Ncirc′ 1 = (Ncirc′ 2) , (4.35)
Nstar′ 1Nstar′ 1 (Nstar′ 2) = (Nstar′ 2) , Ncirc′ 1Ncirc′ 1 (Ncirc′ 2)= Ncirc′ 2, (4.36)
(Nstar′ 2) Nstar′ 1Nstar′ 1 = (Nstar′ 2) , (Ncirc′ 2) Ncirc′ 1Ncirc′ 1 = (Ncirc′ 2) , (4.37)
Nstar′ 2Nstar′ 2 (Nstar′ 1) = (Nstar′ 1) , Ncirc′ 2Ncirc′ 2 (Ncirc′ 1) = (Ncirc′ 1) , (4.38)
Nstar′ 2 (Nstar′ 1) Nstar′ 2 = (Nstar′ 1) , Ncirc′ 2 (Ncirc′ 1) Ncirc′ 2 = (Ncirc′ 1) , (4.39)
(Nstar′ 1) Nstar′ 2Nstar′ 2 = (Nstar′ 1) , (Ncirc′ 1) Ncirc′ 2Ncirc′ 2 = (Ncirc′ 1) . (4.40) 23
So we may observe the following module structures: 1) from (4.35)–(4.37), the sets Nstar′ 2 (Ncirc′ 2) are the middle, right and left ternary modules over Nstar′ 1 (Ncirc′ 1); 2) from (4.38)–(4.40), the set Nstar′ 1 (Ncirc′ 1) are middle, right and left ternary modules over Nstar′ 2 (Ncirc′ 2);
Nstar′ 1Nstar′ 1 (Ncirc′ 1) = (Ncirc′ 1) , (Ncirc′ 1) Nstar′ 1Nstar′ 1 = (Ncirc′ 1) , (4.41)
Nstar′ 1Nstar′ 1 (Ncirc′ 2) = (Ncirc′ 2) , (Ncirc′ 2) Nstar′ 1Nstar′ 1 = (Ncirc′ 2) , (4.42)
Nstar′ 2Nstar′ 2 (Ncirc′ 1) = (Ncirc′ 1) , (Ncirc′ 1) Nstar′ 2Nstar′ 2 = (Ncirc′ 1) , (4.43)
Nstar′ 2Nstar′ 2 (Ncirc′ 2) = (Ncirc′ 2) , (Ncirc′ 2) Nstar′ 2Nstar′ 2 = (Ncirc′ 2) , (4.44)
3) from (4.41)–(4.44), the sets Ncirc′ 1,2 are right and left ternary modules over Nstar′ 1,2;
Ncirc′ 1Ncirc′ 1 (Nstar′ 1) = (Nstar′ 1) , (Nstar′ 1) Ncirc′ 1Ncirc′ 1 = (Nstar′ 1) , (4.45)
Ncirc′ 1Ncirc′ 1 (Nstar′ 2) = (Nstar′ 2) , (Nstar′ 2) Ncirc′ 1Ncirc′ 1 = (Nstar′ 2) , (4.46)
Ncirc′ 2Ncirc′ 2 (Nstar′ 1) = (Nstar′ 1) , (Nstar′ 1) Ncirc′ 2Ncirc′ 2 = (Nstar′ 1) , (4.47)
Ncirc′ 2Ncirc′ 2 (Nstar′ 2) = (Nstar′ 2) , (Nstar′ 2) Ncirc′ 2Ncirc′ 2 = (Nstar′ 2) , (4.48)
4) from (4.45)–(4.48), the sets Nstar′ 1,2 are right and left ternary modules over Ncirc′ 1,2.
D. Group structure of the star and circle 16-vertex matrices
Next we will introduce 8 8 matrices of a special form similar to the star 8-vertex matrices (2.76) and the circle 8-vertex matrices (2.77), analyze their× group structure and establish which ones could be 16-vertex solutions to the ternary braid equations (4.3). We will derive the solutions in the opposite way to that for the 8-vertex Yang-Baxter maps, following the note after (2.34). Indeed, the sum of the permutation bisymm solutions (4.13) gives the shape of the 8 8 star matrix M ′ (as in (2.76)), while × star the sum of symm solutions (4.14) gives the 8 8 circle matrix M ′ (as in (2.77)) × circ x 000000 y 0 z 00 0 0 s 0 0 0 t 0 0 u 0 0 0 0 0 v w 0 0 0 Mstar′ = , (4.49) 0 0 0 a b 0 0 0 0 0 c 0 0 d 0 0 0 f 00 0 0 g 0 h 000000 p x 0000 y 0 0 0 z 0 0 s 0 0 0 0 0 t 000 0 u 0 0 0 v 0 0 w 0 Mcirc′ = , (4.50) 0 f 0 0 g 0 0 0 h 0000 p 0 0 0 0 0 a 0 0 b 0 0 0 c 000 0 d
tr M ′ = x + z + t + v + b + d + g + p, det M ′ = (bv aw)(cu dt)(fs gz)(px hy), (4.51) − − − − 1 1 eigenvalues: d + t 4cu + (d t)2 , d + t + 4cu + (d t)2 , 2 − − 2 − 1 p 1 p 1 b + v 4aw + (b v)2 , b + v + 4aw + (b v)2 , p + x 4hy + (p x)2 , 2 − − 2 − 2 − − 1 p 1 p 1 p p + x + 4hy + (p x)2 , g + z 4fs + (g z)2 , g + z + 4fs + (g z)2 . (4.52) 2 − 2 − − 2 − p p p The 16-vertex matrices are invertible, if det Mstar′ = 0 and det Mcirc′ = 0, which give the following joint conditions on the parameters (cf. (2.79)) 6 6
bv aw =0, cu dt =0, fs gz =0, px hy =0. (4.53) − 6 − 6 − 6 − 6 24
Only in this concrete parametrization (4.49) and (4.50) do the matrices Mstar′ and Mcirc′ have the same trace, determinant and eigenvalues, and they are diagonalizable and conjugate via 10000000 01000000 00100000 00010000 U ′ = . (4.54) 00001010 00000001 00001000 00000100 The matrix U ′ cannot be presented in the form of a triple Kronecker product (4.10), and so two matrices Mstar′ and Mcirc′ are not q-conjugate in the parametrization (4.49) and (4.50), and can lead to different solutions to the ternary braid equations (4.3). It follows from (4.53) that 16-vertex matrices with all nonzero entries equal to 1 are non-invertible, having vanishing determinant and rank 4 (despite each one being a sum of two permutation matrices). In the case all the conditions (4.53) holding, the inverse matrices become p y px hy 00 0 0 00 px hy − g s − − 0 fs gz 0 0 0 0 fs gz 0 − − − 0 0 d 0 0 u 0 0 − cu dt cu dt 0 0 0− b w −0 0 0 1 bv aw bv aw (Mstar′ )− = −a − v− , (4.55) 0 0 0 bv aw bv aw 0 0 0 c − − − t 0 0 cu dt 0 0 cu dt 0 0 f − − − z 0 fs gz 0 0 0 0 fs gz 0 − − − h 00 0 0 00 x − px hy px hy − − p y px hy 0 0 0 0 px hy 0 0 − g s − − 0 fs gz 0 0 fs gz 0 0 0 − − − 0 0 d 0 0 0 0 u − cu dt cu dt 0 0 0− b 0 0 w −0 1 bv aw bv aw (Mcirc′ )− = f − z − − . (4.56) 0 fs gz 0 0 fs gz 0 0 0 h − − − x 0 0 0 0 0 0 − px hy px hy 0− 0 0 a 0− 0 v 0 − bv aw bv aw 0 0 c 0− 0 0− 0 t cu dt − cu dt − − Denoting the sets of matrices corresponding to (4.49) and (4.50) by Mstar′ and Mcirc′ , their multiplications are
Mstar′ Mstar′ = Mstar′ , Mcirc′ Mcirc′ = Mcirc′ , (4.57) and in term of sets Mstar′ = Nstar′ 1 Nstar′ 2 and Mcirc′ = Ncirc′ 1 Ncirc′ 2, and Nstar′ 1 Nstar′ 2 = D and Ncirc′ 1 Ncirc′ 2 = D (see (4.26)). Note that the structure (4.57)∪ is considerably different∪ from the binary case∩ (2.80)–(2.82), and therefo∩re it may not necessarily be related to the Cartan decomposition. The products (4.57) mean that both Mstar′ and Mcirc′ are separately closed with respect to binary matrix multiplication ( ), star circ diag · and therefore 16vert = Mstar′ and 16vert = Mcirc′ are semigroups. We denote their intersection by 8vert = star circS h | ·i S h | ·i S 16vert 16vert which is a semigroup of diagonal 8-vertex matrices. In case, the invertibility conditions (4.53) are fulfilled, S ∩ S star 1 circ 1 the sets M′ and M′ form subgroups = M′ , ( )− , I and = M′ , ( )− , I (where I is star circ G16vert star | · 8 G16vert circ | · 8 8 C the 8 8 identity matrix) of GL (8, ) with the inverseD elements given explicitlyE by (4.55)–(4.56D ). Because the elementsE Mstar′ × star circ and Mcirc′ in (4.49) and (4.50) are conjugates by the invertible matrix U ′ (4.54), the subgroups 16vert and 16vert (as well as the semigroups star and circ ) are isomorphic by the obvious isomorphism G G S16vert S16vert 1 M ′ U ′M ′ U ′− , (4.58) star 7→ circ where U ′ is in (4.54). The “interaction” between Mstar′ and Mcirc′ also differs from the binary case (2.81), because
Mstar′ Mcirc′ = Mquad′ , Mcirc′ Mstar′ = Mquad′ , (4.59)
Mquad′ Mquad′ = Mquad′ , (4.60) 25
where Mquad′ is a set of 32-vertex so called quad-matrices of the form
x1 0 y1 0 0 z1 0 s1 0 t1 0 u1 v1 0 w1 0 a1 0 b1 0 0 c1 0 d1 0 f1 0 g1 h1 0 p1 0 Mquad′ = . (4.61) 0 x2 0 y2 z2 0 s2 0 t2 0 u2 0 0 v2 0 w2 0 a2 0 b2 c2 0 d2 0 f 0 g 0 0 h 0 p 2 2 2 2 Because of (4.60), the set Mquad′ is closed with respect to matrix multiplication, and therefore (for invertible matrices Mquad′ ) quad 1 the group = M′ , ( )− , I is a subgroup of GL (8, C). So, in trying to find higher 32-vertex solutions (having G32vert quad | · 8 at most half as manyD unknown variables asE a general 8 8 matrix) to the ternary braid equations (4.3) it is worthwhile to search within the class of quad-matrices (4.61). × Thus, the group structure of the above 16-vertex 8 8 matrices (4.57)–(4.60) is considerably different to that of 8-vertex × star circ C 4 4 matrices (2.76)–(2.77)as the former contains two isomorphic binary subgroups 16vert and 16vert of GL(8, ) (cf. (2.80)–(2.82)× and (4.57)). G G The sets Mstar′ , Mcirc′ and Mquad′ are closed with respect to matrix addition as well, and therefore (because of the distributivity C star circ quad of ) they are the matrix rings 16vert, 16vert and 32vert, respectively. In the invertible case (4.53) and det Mquad′ = 0, these become matrix fields. R R R 6
E. Pauli matrix presentation of the star and circle 16-vertex constant matrices
The main peculiarity of the 16-vertex 8 8 matrices (4.57)–(4.60) is the fact that they can be expressed as special tensor (Kronecker) products of the Pauli matrices (see,× also, [18, 27]). Indeed, let Σ = ρ ρ ρ , i, j, k =1, 2, 3, 4, (4.62) ijk i ⊗K j ⊗K k where ρi are Pauli matrices (we have already used the letter “σ” for the braid group generators (2.5)) 0 1 0 i 1 0 1 0 ρ = , ρ = , ρ = , ρ = I = . (4.63) 1 1 0 2 i −0 3 0 1 4 2 0 1 − Among the total of 64 8 8 matrices Σ (4.62) there are 24 which generate M ′ (4.49) and M ′ (4.50): × ijk star circ 8 diagonal matrices: Σdiag = Σ , Σ , Σ , Σ , Σ , Σ , Σ , Σ ; • { 333 334 343 344 433 434 443 444} 8 anti-diagonal matrices: Σadiag = Σ , Σ , Σ , Σ , Σ , Σ , Σ , Σ ; • { 111 112 121 122 211 212 221 222} 8 circle-like matrices (Mcirc′ with 0’s on diagonal): Σcirc = Σ131, Σ132, Σ141, Σ142, Σ231, Σ232, Σ241, Σ242 . Thus,• in general we have the following set structure for the star{ and circle 16-vertex matrices (4.49) and (4.50)}
M′ = Σdiag Σadiag, (4.64) star ∪ M′ = Σdiag Σcirc, (4.65) circ ∪ M′ M′ = Σdiag. (4.66) star ∩ circ In particular, for the 8-vertex permutation solutions (4.13)–(4.14) of the ternary braid equations (4.3) we have 1 c˜bisymm1,2 = (Σ +Σ Σ Σ ) , (4.67) rank=8 2 111 444 ± 212 ± 343 1 c˜symm1,2 = (Σ +Σ Σ Σ ) . (4.68) rank=8 2 141 444 ± 232 ± 333
The non-invertible 16-vertex solutionsMstar′ (4.49) and Mcirc′ (4.50) having 1’s on nonzero places are of rank = 4 and can be presented by (4.62) as follows 10000001 01000010 00100100 00011000 Mstar′ (1) = =Σ111 +Σ444, (4.69) 00011000 00100100 01000010 10000001 26
10000100 01001000 00100001 00010010 Mcirc′ (1) = =Σ141 +Σ444. (4.70) 01001000 10000100 00010010 00100001 Similarly, one can obtain the Pauli matrix presentation for the general star and circle 16-vertex matrices (4.49) and (4.50) which will contain linear combinations of the 16 parameters as coefficients before the Σ’s.
F. Invertible and non-invertible 16-vertex solutions to the ternary braid equations
First, consider the 16-vertex solutions to (4.3) having the star matrix shape (4.49). We found the following 2 one-parameter invertible solutions
x3 000 0 0 0 1 0 x3 00 0 0 x2 −0 3 2 ∓ 0 0 x 0 0 x 0 0 3 3 4 − trc ˜ =8x , 16 vert,star 0 0 0 x x 0 0 0 24 c˜ − (x)= , detc ˜ = 16x , x =0, (4.71) rank=8 2 ∓ 3 6 0 0 0 x x 0 0 0 3 [4] 3 [4] 4 ± 3 eigenvalues: (1 + i)x , (1 i)x . 0 0 x 0 0 x 0 0 − 4 3 0 x 00 0 0 x 0 x6 ±000 0 0 0 x3 Both matrices in (4.71) are diagonalizable and are conjugates via
1 0 0 0 0000 0 10 0 0000 0− 0 1 0 0000 0 0 0 10000 Ustar = − , (4.72) 0 0 0 0 1000 0 0 0 0 0100 0 0 0 0 0010 0 0 0 0 0001 which cannot be presented in the form of a triple Kronecker product (4.10). Therefore, the two solutions in (4.71) are not q-conjugate and become different 16-vertex one-parameter invertible solutions of the braid equations (4.3). In search of 16-vertex solutions to the total braid equations (4.3) of the circle matrix shape (4.50) we found that only non- invertible ones exist. They are the following two 2-parameter solutions of rank 4
xy 0 0 0 0 y2 0 0 ±0 xy 0 0 xy 0 0 0 0± 0 xy 0 0 0 0 y2 ± 16 vert,circ 0 0 0 xy 0 0 xy 0 trc ˜ = 8xy, c˜rank− =4 (x, y)= ± , ± [4] [4] (4.73) 0 xy 0 0 xy 0 0 0 eigenvalues: 2xy , 0 . 2 ± { } { } x 0 0 0 0 xy 0 0 ± 0 0 0 xy 0 0 xy 0 0 0 x2 0 0 0± 0 xy ± Two matrices in (4.73) are not even conjugates in the standard way, and so they are different 16-vertex two-parameter non- invertible solutions to the braid equations (4.3). 27
For the only partial 13-braid equation (4.5), there are 4 polynomial 16-vertex two-parameter invertible solutions x 0 0 00 y2 0 0 x 0 0 00 y2 0 0 0 xy 0 0 x 0 0 0 0 xy 0 0 x 0 0 0 0 0 x 0 00 0 y2 0 0 x 0− 000 y2 ± ± 16 vert,13circ 00 0 xy 0 0 x 0 0 0 0 xy 0 0 x 0 c˜rank− =8 (x, y)= ± , ∓ , (4.74) 0 x 0 0 xy 0 0 0 0 x 0 0 xy 0 0 0 2 2 − x 0 0 00 x 0 0 x 0 0 00 x 0 0 00 0 x 0 0 xy 0 0 0 0 x 0 0 xy 0 0 0 x2 ±0 00 0 x 0 0 x2 ∓0 000 x ± ± 4 trc ˜ =4x (y + 1) , detc ˜ = x8 y2 1 , x =0,y =1, eigenvalues: x (y + 1) [4] , x (y 1) [2] , x (y 1) [2] . − 6 6 { } { − } {− − } (4.75) Also, for the partial 13-braid equation (4.5), we found 4 exotic irrational (an analog of (2.88) for the Yang-Baxter equation (2.12)) 16-vertex, two-parameter invertible solutions of rank 8 of the form 16 vert,13circ,1 c˜rank− =8 (x, y) x(2y 1)0 0 0 0 y2 0 0 − 0 xy 0 0 x 2(y 1)y +10 0 0 0 0 x(2y 1) 0− 0 0 0 y2 − p ± 0 0 0 xy 0 0 x 2(y 1)y +1 0 = ± − , 0 x 2(y 1)y +10 0 xy 0 0 0 p x2 −00 0 0 x 0 0 p 0 0 0 x 2(y 1)y +1 0 0 xy 0 0 0 x2 ± 0− 000 x ± p (4.76)
16 vert,13circ,2 c˜rank− =8 (x, y) x(2y 1)0 0 0 0 y2 0 0 − 0 xy 0 0 x 2(y 1)y +10 0 0 0 0 x(2y 1) 0− 0− 0 0 y2 − p ± 0 0 0 xy 0 0 x 2(y 1)y +1 0 = ∓ − , 0 x 2(y 1)y +10 0 xy 0 0 0 p x2 − 0− 0 0 0 x 0 0 p 0 0 0 x 2(y 1)y +1 0 0 xy 0 0 0 x2 ∓ 0− 000 x ± p (4.77)
trc ˜ =8xy, detc ˜ = x8 (y 1)8 , x =0, y =1, (4.78) − 6 6 [4] [4] eigenvalues: x y + 2(y 1)y +1 , x y 2(y 1)y +1 . (4.79) − − − The matrices in (4.74)–(4.77) are diagonalizable,n p have the sameo eigenvaluesn (4.79)p and are pairwiseo conjugate by 10 0 0 0000 01 0 0 0000 0 0 1 0 0000 − 00 0 10000 Ucirc = − . (4.80) 00 0 0 1000 00 0 0 0100 00 0 0 0010 00 0 0 0001 Because Ucirc cannot be presented in the form (4.10), all solutions in (4.74)–(4.77) are not mutually q-conjugate and become 8 different 16-vertex two-parameter invertible solutions to the partial 13-braid equation (4.5). If y = 1, then the matrices (4.74)– (4.77) become of rank 4 with vanishing determinants (4.75), (4.78), and therefore in this case they are a 16-vertex one-parameter circle of non-invertible solutions to the total braid equations (4.3). Further families of solutions could be constructed using additional parameters: the scaling parameter t in (4.8) and the complex elements of the matrix q (4.9). 28
n G. Higher 2 -vertex constant solutions to n-ary braid equations
Next we considered the 4-ary constant braid equations (3.4)–(3.6) and found the following 32-vertex star solution 100000000 0 0 0 0 0 0 1 010000000 0 0 0 0 0 1− 0 001000000 0 0 0 0 10− 0 − 000100000 0 0 0 10 0 0 00001000 0 0 0 10− 0 0 0 00000100 0 0 10− 00 0 0 00000010 0 1000000− 00000001 10000000− c˜16 = − . (4.81) 000000011 0 0 0 0 0 0 0 000000100 1 0 0 0 0 0 0 000001000 0 1 0 0 0 0 0 000010000 0 0 1 0 0 0 0 000100000 0 0 0 1 0 0 0 001000000 0 0 0 0 1 0 0 010000000 0 0 0 0 0 1 0 100000000 0 0 0 0 0 0 1 We may compare (4.81) with particular cases of the star solutions to the Yang-Baxter equation (2.86) and the ternary braid equation (4.71) 10000 0 0 1 0100 0 0 1− 0 10 0 1 0010 0 10− 0 − − 0 1 1 0 0001 10 0 0 c˜4 = − , c˜8 = − . (4.82) 01 1 0 00011 0 0 0 10 0 1 00100 1 0 0 01000 0 1 0 10000 0 0 1 Informally we call such solutions the “Minkowski” star solutions, since their legs have the “Minkowski signature”. Thus, we assume that in the general case for the n-ary braid equation there exist 2n+1-vertex 2n 2n matrix “Minkowski” star invertible solutions of the above form × 1000 0 1 . . − 0 .. 0 0 .. 0 0 0 1 10 0 c˜2n = − . (4.83) 0011 0 0 . . 0 .. 0 0 .. 0 1000 0 1 This allows us to use the general solution (4.83) as n-ary braiding quantum gates with an arbitrary number of qubits.
V. INVERTIBLE AND NONINVERTIBLE QUANTUM GATES
Informally, quantum computing consists of preparation (setting up an initial quantum state), evolution (by a quantum circuit) and measurement (projection onto the final state). Mathematically (in the computational basis) the initial state is a vector in a Hilbert space (multi-qubit state), the evolution is governed by successive (quantum circuit) invertible linear transformations (unitary matrices called quantum gates) and the measurement is made by non-invertible projection matrices to leave only one final quantum (multi-qubit) state. So, quantum computing is non-invertible overall, and we may consider non-invertible transfor- mations at each step. It was then realized that one can “invite” the Yang-Baxter operators (solutions of the constant Yang-Baxter equation) into quantum gates , providing a means of entangling otherwise non-entangled states. This insight uncovered a deep connection between quantum and topological computation (see for details, e.g. [9, 13]). Here we propose extending the above picture in two directions. First, we can treat higher braided operators as higher braiding gates. Second, we will analyze the possible role of non-invertiblelinear transformations (described by the partial unitary matrices 29 introduced in (2.20)–(2.21)), which can be interpreted as a property of some hypothetical quantum circuit (for instance, with specific “loss” of information, some kind of “dissipativity” or “vagueness”). This can be considered as an intermediate case between standard unitary computing and the measurement only computing of [51]. To establish notation recall [1], that in the computational basis (vector representation) and Dirac notation, a (pure) one-qubit state is described by a vector in two-dimensional Hilbert space V = C2
1 0 ψ ψ(1) = a 0 + a 1 , 0 = , 1 = , a 2 + a 2 =1, a C, ,i =1, 2, (5.1) | i≡ 0 | i 1 | i | i 0 | i 1 | 0| | 1| i ∈ E where ai is a probability amplitude of i . Sometimes, for a one-qubit state it is convenient to use the Bloch unit sphere representation (normalized up to a general| i unimportant and unmeasurable phase)
θ θ ψ (θ,γ) = cos 0 + eiγ sin 1 , 0 θ π, 0 γ 2π. (5.2) | i 2 | i 2 | i ≤ ≤ ≤ ≤
A (pure) state of L-qubits ψ(L) is described by 2L amplitudes, and so is a vector in 2L-dimensional Hilbert space. If ψ(L) cannot be presented as a tensor product of L one-qubit states (5.1), it is called entangled. For instance, a two-qubit pure state
ψ(2) = a 00 + a 01 + a 10 + a 11 , a 2 + a 2 + a 2 + a 2 =1, a C, ,i,j =1, 2, (5.3) 00 | i 01 | i 10 | i 11 | i | 00| | 01| | 10| | 11| ij ∈ E is entangled, if det (a ) =0, and the concurrence ij 6 C(2) C(2) ψ(2) =2 det (a ) (5.4) ≡ | ij | E is the measure of entanglement 0 C(2) 1. It follows from (5.1), that the tensor product of states has vanishing concurrence C(2) ( ψ ψ )=0. An example≤ of the≤ maximally entangled (C(2) =1) two-qubit states is the (first) Bell state ψ(2) = | 1i ⊗ | 2i Bell √ . ( 00 + 11 )/ 2 | Thei concurrence| i of the three-qubit state
1 1 ψ(3) = a ijk , a 2 =1, a C, (5.5) ijk | i | ijk| ijk ∈ E i,j,k=0 i,j,k=0 X X is determined by the Cayley’s 2 2 2 hyperdeterminant × × C(3) =4 h det (a ) , 0 C(3) 1, (5.6) | ijk | ≤ ≤
h det (a )= a2 a2 + a2 a2 + a2 a2 + a2 a2 2a a a a ijk 000 111 001 110 010 101 100 011 − 000 001 110 111 2a a a a 2a a a a 2a a a a 2a a a a − 000 010 101 111 − 000 011 100 111 − 001 010 101 111 − 001 011 100 110 2a a a a +4a a a a +4a a a a . (5.7) − 010 011 100 101 000 011 101 110 001 010 100 111 Thus, if the three-qubit state (5.5) is not entangled, then C(3) = 0 (for the tensor product of one-qubit states). One of the maximally entangled ( (3) ) three-qubit states is the GHZ state (3) √ . C =1 ψ GHZ = ( 000 + 111 )/ 2 | i | L i L A quantum L-qubit gate is a linear transformation of 2L-dimensional Hilbert space C2 ⊗ C2 ⊗ which in the com- → putational basis (5.1) is described of the 2L 2L matrix U (L) such that the L-qubit state transforms as ψ (L) = U (L) ψ(L) . ′ In this way, a quantum circuit is described as× the successive application of elementary gates to an initial quantum state, that is the product of the corresponding matrices (for details, see, e.g., [1]). It is a standard assumption that each elementary L -qubit transformation is unitary, which implies the following strong restriction on the corresponding matrix U U (L) as ≡ ⋆ ⋆ U U = UU = I I2L 2L , (5.8) ≡ × where I is the 2L 2L identity matrix for L-qubit state and the operation (⋆) is the conjugate-transposition. The first equality in (5.8) means that× the matrix U (L) is normal (cf. (2.20)–(2.21)). The equations (5.8) follow from the definition of the adjoint operator
⋆ Uψ(L) Iϕ(L) = Iψ(L) U ϕ(L) (5.9) | | D E D E 30
L applied to this simplest example of L-qubits in the 2L-dimensional Hilbert space C2 ⊗ (for the general case the derivation almost literally coincides), which we write in the following special form (in Dirac notation with bra- and ket- vectors) with explicitly added identities. Then (5.8) follows from (5.9) as
⋆ ⋆ U Uψ(L) Iϕ(L) = Iψ(L) UU ϕ(L) = Iψ(L) Iϕ(L) , (5.10) | | | D E D E D E and any unitary matrix preserves the inner product
Uψ(L) Uϕ(L) = Iψ(L) Iϕ(L) , (5.11) | | D E D E which means that unitary operators satisfying (5.8) are bounded operators (bounded matrices in our case) and invertible with the 1 ⋆ inverse U − = U . Let us consider a possibility of non-invertible intermediate transformations of L-qubit states, i.e. non-invertible gates which are described by the 2L 2L matrices U (r) of (possibly) less than full rank 1 r 2L. This can be related to the production of “degenerate” states (see,× e.g. [42]), “particle loss” [52–54], and the role of ranks≤ in≤ multiparticle entanglement [55, 56]. In the limited cases U r =2L U = U (L), and U (1) corresponds to the measurement matrix being the projection to one ≡ final vector i . In this case, for non-invertible transformations with r < 2L instead of unitarity (5.8) we consider partial final unitarity (2.20)–(2.21)| i as
⋆ U (r) U (r)= I1 (r) , (5.12) ⋆ U (r) U (r) = I2 (r) , (5.13) where I1 (r) and I2 (r) are (or may be) different partial shuffle identities having r units on the diagonal. There is an exotic limiting case, which is impossible for the identity I: we call two partial identities orthogonal, if
I1 (r) I2 (r)= Z, (5.14)
L L where Z = Z2L 2L is the zero 2 2 matrix. × × ⋆ We propose corresponding non-invertible analogs of (5.9)–(5.11) as follows. The partial adjoint operator U (r) in the L 2L-dimensional Hilbert space C2 ⊗ is defined by