 
  
  
  
  
 
It may seem a little surprising that a very small anisotropy can lead to a 
substantially high  .  This may be explained by the following argument. 
At low T, the spins are highly correlated in the isotropic case.  Since no 
direction is preferred, the correlated spins fluctuate in all directions, 
resulting in zero net magnetization.  Adding a very small anisotropy into the 
system introduces a preferred direction, so that the already highly 
correlated spins will fluctuate around this direction, leading to a global 
magnetization.
.  This may be explained by the following argument. 
At low T, the spins are highly correlated in the isotropic case.  Since no 
direction is preferred, the correlated spins fluctuate in all directions, 
resulting in zero net magnetization.  Adding a very small anisotropy into the 
system introduces a preferred direction, so that the already highly 
correlated spins will fluctuate around this direction, leading to a global 
magnetization.
More quantitatively, the crossover from the isotropic Heisenberg behavior to 
the Ising behavior occurs at  , where the correlation length is of 
order of some power of the inverse anisotropy.  From the scaling
arguments [Riedel:69a],
, where the correlation length is of 
order of some power of the inverse anisotropy.  From the scaling
arguments [Riedel:69a],  where
where  is the crossover exponent.  In the two-dimensional model, both
 is the crossover exponent.  In the two-dimensional model, both 
 and
 and  are infinite, but the ratio is approximately 1/2.  For
 are infinite, but the ratio is approximately 1/2.  For
 , this relation indicates that the Ising behavior is valid for
, this relation indicates that the Ising behavior is valid for 
 , which is clearly observed in Figure 6.16.  
Similar crossover around
, which is clearly observed in Figure 6.16.  
Similar crossover around  for
 for  is also 
observed in Figure 6.16.  At low T, for the isotropic quantum 
model, the correlation length behaves as [Ding:90g]
 is also 
observed in Figure 6.16.  At low T, for the isotropic quantum 
model, the correlation length behaves as [Ding:90g] 
 where
 where  .  Therefore, 
we expect
.  Therefore, 
we expect 
where  is spin-S dependent constant of order one.
Therefore, even a very small anisotropy
 is spin-S dependent constant of order one.
Therefore, even a very small anisotropy  will induce a phase
transition  at a substantially high temperature
(
 will induce a phase
transition  at a substantially high temperature
( ).  This crude picture, suggested a long time ago to
explain the observed phase transitions, is now confirmed by the
extensive quantum Monte Carlo  simulations for the
first time.  Note that this problem is an extreme case both because it
is an antiferromagnet (more difficult to become ordered than the
ferromagnet), and because it has the largest quantum fluctuations
(spin-
).  This crude picture, suggested a long time ago to
explain the observed phase transitions, is now confirmed by the
extensive quantum Monte Carlo  simulations for the
first time.  Note that this problem is an extreme case both because it
is an antiferromagnet (more difficult to become ordered than the
ferromagnet), and because it has the largest quantum fluctuations
(spin- ).  Since
).  Since  varies slowly with h, we can
estimate
 varies slowly with h, we can
estimate  at
 at  :
:

 
 
  
  
  
 