Chemistry Reference
In-Depth Information
2.2.1 Pitfall in Transforming Trio Strength Between Lattice-Gas
and Ising Models
Many researchers recast the lattice-gas model into an Ising model before doing
computations. This seemingly innocent procedure invites pitfalls when multisite
interactions are involved. Here we offer a particular example: what seems like a
relatively modest three-spin interaction can correspond to an unphysically large trio
interaction in the lattice-gas Hamiltonian. Our example involves a square lattice
with M
2 (first and second neighbor pair interactions) and the right-triangle trio
E RT corresponding to two E 1 legs at right angles and an E 2 hypotenuse (or E 112 for
short, in a general formal notation [ 3 ]).
The mapping to spin language, with s i
=
1, is n i
= (
1
+
s i )/
2. We see
E 1
4 +
E 2
4 +
E RT
2
E RT
4
E RT
8
H =
s i s j +
s i s j +
s i s j s k
(2.3)
ij
ij
ijk
1
2
RT
In Ising or spin language, the three coefficients are called
J 1 ,
J 2 , and
J RT ,
respectively. For the pair interactions, we easily see that
J 2
J 1 =
E 2 /
E 1 +
E RT /
E 1
E 2
E 1
E RT |
for
|
4
|
E 1 |
(2.4)
1
+
2 E RT /
E 1
One might then naively - but incorrectly - expect that J RT /
J 1
E RT /
E 1 . Instead
J RT
J 1 =
E RT /
E 1
E RT
E 1 =
2 J RT /
J 1
(2.5)
2
+
4 E RT /
E 1
1
4 J RT /
J 1
J 1
This highly non-linear relation leads to a surprising result: For J RT /
1
/
4,
E 1
becomes large and negative. A similar effect would occur in the opposite direction
for E RT /
E RT /
E 1
J RT /
J 1 . Furthermore, if J RT /
J 1 increases to slightly above 1/4, E RT /
2, a larger magnitude than one is likely to encounter.
Finally, it is unfortunate (to say the least) that some researchers (including promi-
nent ones) denote the lattice-gas energy parameters as J . Even in the simplest case
of just a nearest-neighbor interaction, the lattice-gas energy differs from the Ising
energy by a factor of 4; thus, misinterpretation and numerical inaccuracies are very
likely.
E 1 ≈−
1
/
2.2.2 Effect on Phase Boundaries: Asymmetries Not Inevitable
A trio interaction, which breaks particle-hole symmetry (or up-down symmetry in
the Ising viewpoint), is generally expected to lead inevitably to substantial asymme-
tries in phase diagrams about half-monolayer coverage. A rather surprising finding
of numerical [Monte Carlo] calculations is that a single type of trio interaction need
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