
collisions with a left or right wall the rapidity
variable changes from p to p and back. In most
examples, in which the rapidities are difference
variables such that R(p, q) = R(p q), one also has
p = p,with some constant. The corresponding
left boundary weights are K
(p, p) satisf ying
ˇ
K
1
ðq; qÞ
ˇ
R
12
ðp; qÞ
ˇ
K
1
ðp; pÞ
ˇ
R
12
ðq; pÞ
¼
ˇ
R
12
ðp; qÞ
ˇ
K
1
ðp; pÞ
ˇ
R
12
ðq; pÞ
ˇ
K
1
ðq; qÞ½29
with
ˇ
K
1
(p, p) de fined by a direct product as in [24]
appending unit matrices for positions i52, and a
similar equation must hold for the right boundary.
Most work has been done for vertex models, while
Pearce and co-workers wrote several papers on the
IRF-model version.
Higher-Dimensional Generalizations
In 1980 Zamolodchikov introduced a three-
dimensional generalization of the YBE, the so-called
tetrahedron equations (TEs), and he found a special
solution. Baxter then succeeded in proving that
this solution satisfies all TEs. Baxter and Bazhanov
showed in 1992 that this solution can be seen as
a special case of the sl(1) chiral Potts model.
Several authors found furth er generalizations more
recently.
Inversion Relations
When !
(p, p) /
, that is, the weight decouples
when the two rapidities are equal, one can derive the
local inverse relati on depicted in Figure 15, which is
a generalization of the Reidemeister move of type II
in Figure 4. It is easily shown that C(q, p) = C(p, q).
This local relatio n implies also a global inversion
relation which can be found in many ways. The
following heuristic way is the easiest: consider the
situation in Figure 16, with N closed p-rapidity lines
and M closed q-rapidity lines. For M and N large,
we may expect the partition function of Figure 16
to factor asymptotically in top- and bottom-half
contributions. If each line segment carries a state
variable that can assume Q values, then the total
partition function factors by repeated application of
the relation in Figure 15 into the contribution of
M þ N circles. Therefore,
Z ¼ Q
MþN
Cðp; qÞ
MN
Z
M; N
ðp; q ÞZ
N; M
ðq; pÞ½30
Taking the thermodynamic limit,
zðp; qÞ lim
M; N!1
Z
M; N
ðp; q Þ
1=MN
½31
one finds
zðp; qÞzðq; pÞ¼Cðq; pÞ½32
In many models, eqn [32], supplemented with some
suitable symmetry and analyticity conditions, can be
used to calculate the free energy per site.
See also: Affine Quantum Groups; Bethe Ansatz;
Classical r-matrices, Lie Bialgebras, and Poisson Lie
Groups; Eight Vertex and Hard Hexagon Models; Hopf
Algebras and q-Deformation Quantum Groups;
Integrability and Quantum Field Theory; Integrable
Discrete Systems; Integrable Systems: Overview; The
Jones Polynomial; Knot Invariants and Quantum Gravity;
Knot Theory and Physics; Sine-Gordon Equation;
Topological Knot Theory and Macroscopic Physics;
Two-Dimensional Ising Model; von Neumann Algebras:
Subfactor Theory.
Further Reading
Au-Yang H and Perk JHH (1989) Onsager’s star-triangle
equation: master key to integrability. Advanced Studies in
Pure Mathematics 19: 57–94.
Baxter RJ (1982) Exactly Solved Models in Statistical Mechanics.
London: Academic Press.
qp pq
C(p,q)
=
Figure 15 Local inversion relation.
p
p
p
p
qqqqqq
p
p
p
p
Figure 16 Heuristic derivation of inversion relation.
472 Yang–Baxter Equations