Introduction to Landau-Ginzberg theory next up previous
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Introduction to Landau-Ginzberg theory

The Landau-Ginzberg (LG) theory is a phenomenological theory meant to be used only near the critical point. Thus, it is formulated as a macroscopic theory. The basic idea of LG theory is to introduce a spin density field variable tex2html_wrap_inline600 defined by

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Then the total magnetization is given by

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Since the free energy at zero field is A=A(N,M,T), there should be a corresponding free energy density tex2html_wrap_inline604 such that

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It is assumed that tex2html_wrap_inline606 can be represented as a power series according to

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such that tex2html_wrap_inline608 and tex2html_wrap_inline610 are both positive for tex2html_wrap_inline612 and tex2html_wrap_inline608 vanishes at tex2html_wrap_inline582 . These conditions are analogous to those exhibited by the total free energy in MFT above and near the critical point (see previous lecture). By symmetry, all odd terms vanish and are, therefore, not explicitly included.

In the presence of a magnetic field tex2html_wrap_inline618 , we have a Gibbs free energy density given by

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In addition, a term tex2html_wrap_inline620 with tex2html_wrap_inline622 is added to the free energy in order to damp out local fluctuations. If there are significant local fluctuations, then tex2html_wrap_inline624 becomes large, so these field configurations contribute negligibly to the partition function, which is defined by

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Thus, the LG theory is a field theory. The form of this field theory is well known in quantum field theory, and is known as a d-dimensional scalar Klein-Gordon theory. In terms of Z, a correlation function at zero field can be defined by

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Thus, by studying the behavior of the correlation function, the exponents tex2html_wrap_inline552 and tex2html_wrap_inline554 can be determined.

For the choice tex2html_wrap_inline634 , the theory can be solved exactly analytically. This is known as the Gaussian model, for which

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which leads to values of tex2html_wrap_inline554 and tex2html_wrap_inline552 of 0 and 1/2, respectively. These values are known as the ``classical'' exponents. They are independent of the number of spatial dimensions d. Dependence on d comes in at higher orders in S. Comparing these to the exact exponents from the Onsager solution, which gives tex2html_wrap_inline646 and tex2html_wrap_inline648 , it can be seen that the classical exponents are only qualitatively correct. Going to higher orders in the theory leads to improved results, although the theory cannot be solved exactly analytically. It can either be solved numerically using path integral Monte Carlo or Molecular Dynamics or analytically perturbatively using Feynman diagrams.


next up previous
Next: Renormalization group and the Up: No Title Previous: The exponents and

Mark Tuckerman
Tue May 4 17:17:42 EDT 1999