RGApproachToInteractingFermions: Difference between revisions

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where the action <math>S</math> is
where the action <math>S</math> is
<math> \displaystyle S=\int_{0}^{\beta}{d\tau \left [\sum_{\bf r}{\psi^{\ast}({\bf r},\tau)\left (\frac{\partial}{\partial\tau}-\mu\right )\psi({\bf r},\tau)+H[\psi^{\ast},\psi]}\right ]}</math>
and <math>H[\psi^{\ast},\psi]</math> is the Hamiltonian in normal-ordered form with all the bosonic (fermionic) creation and annihilation operators replaced with complex (Grassman) numbers.  Note that we are considering a theory on some underlying lattice, so that <math>{\bf r}</math> is the position vector for a point on the lattice.


=System at half-filling in one dimension=
=System at half-filling in one dimension=

Revision as of 14:59, 30 November 2010

Introduction

The renormalization group (RG) is a very powerful tool in physics. Essentially, it is a way to continuously map a given theory onto other theories possessing the same low-energy physics by successively integrating out "fast", or high-energy, modes. This is expressed in terms of differential equations giving the "flows" of different coupling constants that appear in the theory.

The basic proceedure is as follows. Let us consider a given interacting Hamiltonian, and write the associated partition function in path integral form:

where the action is

and is the Hamiltonian in normal-ordered form with all the bosonic (fermionic) creation and annihilation operators replaced with complex (Grassman) numbers. Note that we are considering a theory on some underlying lattice, so that is the position vector for a point on the lattice.

System at half-filling in one dimension

System with spherically symmetric Fermi surface in two or three dimensions

System with non-spherically symmetric Fermi surface in two dimensions

System with nested Fermi surface in two dimensions