Mean field models: Difference between revisions

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(it corresponds to a maximum in energy), whereas two others are stable. Slightly below <math>T_c</math>,
(it corresponds to a maximum in energy), whereas two others are stable. Slightly below <math>T_c</math>,
:<math>\bar{s} =\pm\sqrt{3\left(1 - \frac{T}{T_c}\right)}. </math>
:<math>\bar{s} =\pm\sqrt{3\left(1 - \frac{T}{T_c}\right)}. </math>
==General discussion==
The solution obtained shares a number of features with any other mean field approximation:
*It largely ignores geometry, which may be important in some cases. In particular, it reduces the lattice details to just the number of neighbours.
*As a consequence, it may predict phase transitions where none are found: the [[1-dimensional_Ising_model|1-D ising model]] <math>n=2</math> is known to lack any phase transition (at finite temperature)
*In general, the theory ''underestimates fluctuations''
*It also leads to ''classical critical exponents'', like the <math>\left(1 - \frac{T}{T_c}\right)^{1/2}</math> decay above. In 3-D, the magnetization follows a power law with a different exponent.
*Nevertheless, above a certain space dimension the critical exponents are correct. This dimension is 4 for the Ising model, as predicted by a self-consistency requirement due to E.M. Lipfshitz (similar ones are due to Peierls and L.D. Landau)

Revision as of 15:26, 3 May 2010

A mean field model, or a mean field solution of a model, is an approximation to the actual solution of a model in statistical physics. The model is made exactly solvable by treating the effect of all other particles on a given one as a mean field (hence its name). It appear in different forms and different contexts, but all mean field models have this feature in common.

Mean field solution of the Ising model

A well-known mean field solution of the Ising model, known as the Bragg-Williams approximation goes as follows. From the original Hamiltonian,

suppose we may approximate

where is the number of neighbors of site (e.g. 4 in a 2-D square lattice), and is the (unknown) magnetization:

Therefore, the Hamiltonian turns to

as in the regular Langevin theory of magnetism: the spins are independent, but coupled to a constant field of strength

The magnetization of the Langevin theory is

Therefore:

This is a self-consistent expression for . There exists a critical temperature, defined by

At temperatures higher than this value the only solution is . Below it, however, this solution becomes unstable (it corresponds to a maximum in energy), whereas two others are stable. Slightly below ,

General discussion

The solution obtained shares a number of features with any other mean field approximation:

  • It largely ignores geometry, which may be important in some cases. In particular, it reduces the lattice details to just the number of neighbours.
  • As a consequence, it may predict phase transitions where none are found: the 1-D ising model is known to lack any phase transition (at finite temperature)
  • In general, the theory underestimates fluctuations
  • It also leads to classical critical exponents, like the decay above. In 3-D, the magnetization follows a power law with a different exponent.
  • Nevertheless, above a certain space dimension the critical exponents are correct. This dimension is 4 for the Ising model, as predicted by a self-consistency requirement due to E.M. Lipfshitz (similar ones are due to Peierls and L.D. Landau)