Feynman rules for nonlinear sigma models

In summary, nonlinear sigma models are field theories with fields constrained to a nontrivial manifold, making it impossible to use standard perturbation theory methods. To overcome this, the Faddeev-Popov procedure is used to convert the functional integral over the constrained fields into an integral over unconstrained fields, including new auxiliary fields. This method is well-known in YM theories, where the introduction of ghost and anti-ghost fields is necessary to preserve unitarity. The CP(N-1) model, which also has a constrained field, can be quantized using this method by introducing two auxiliary fields. The resulting effective action is a functional of these fields and the interactions between the original fields generate a gauge field, confining the original degrees of
  • #1
hyperkahler
2
0
Nonlinear sigma models are particular field theories in which the fields take values in some nontrivial manifold. In the simplest cases this is equivalent to saying that the fields appearing in the lagrangian are subject to a number of constraints. Since the lagrangian fields are not independent from one another they cannot be used directly to construct Feynman diagrams in perturbation theory. The most general way to deal with the quantization of constrained systems is by use of the Faddeev-Popov procedure. The functional integral over the constrained set of fields is converted to a functional integral over unconstrained fields, the unconstrained fields including now, in addition to the original fields, also new auxiliary fields. The basic idea is to exponentiate the constraint, converting it to new lagrangian terms through the introduction of new fields. In YM theories this quantization procedure is well-known and leads to the appearance of so called ghost and anti-ghost fields: by imposing a gauge fixing condition, for example a Lorentz-gauge condition, one ends up with new scalar but anticommuting fields in the adjoint representation of the gauge group. These fields cannot appear as external states, since they violate the spin-statistics theorem, but must be included as internal propagating particles to preserve unitarity.

I was thinking about how to implement a similar idea for nonlinear sigma models so that standard perturbation theory methods via Feynman diagrams are applicable. In particular consider the [itex]CP(N-1)[/itex] model:

[tex]
L= \frac{2}{g^2}[(\partial_\mu n^{\dagger})(\partial^\mu n)+(n^\dagger \partial_\mu n)^2]
[/tex]

where [itex] n [/itex] is a N-component vector of complex scalars with the constrained [itex] n^\dagger n=1 [/itex]. My problem is that this constraint leads to a new lagrangian term [itex] \lambda(n^\dagger n-1) [/itex] (introducing an auxiliary field [itex] \lambda [/itex] as lagrangian multiplier). The new field however is non propagating. Is there any way to correct this or do you know any other way how to quantize this type of system?
 
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  • #2
The solution of the ##CP^{N-1}## model in 2d is discussed in the 2nd to last chapter of Coleman's Aspects of Symmetry. The idea is to introduce 2 auxiliary fields. The first is a vector ##A_\mu## that you use to rewrite the quartic term ##(n^\dagger\partial_\mu n)^2## term. The second is ##\sigma## which is the same as your ##\lambda##, imposing the constraint. The resulting action is quadratic in ##n##, so you can integrate ##n## out to give an effective action which is a functional of the auxiliary fields. The graphic expansion is in powers of ##1/N##.

The physical interpretation of the result is that the interactions between the ##n## dynamically generate a gauge field ##A_\mu##. The resulting long-range interaction is linear and so the original ##n## degrees of freedom are confined.
 

1. What are the Feynman rules for nonlinear sigma models?

The Feynman rules for nonlinear sigma models are a set of mathematical rules that are used to calculate the probability amplitudes for interactions between particles in a field theory. They were developed by physicist Richard Feynman and are based on the principles of quantum field theory.

2. How are the Feynman rules used in nonlinear sigma models?

The Feynman rules are used to calculate the scattering amplitudes for particles in a nonlinear sigma model. These amplitudes represent the probabilities of different particle interactions and can be used to make predictions about the behavior of the system.

3. What are the advantages of using Feynman rules in nonlinear sigma models?

Using Feynman rules in nonlinear sigma models allows for a systematic and efficient way to calculate scattering amplitudes, making it easier to make predictions about the behavior of the system. It also allows for the incorporation of higher order corrections, making the calculations more accurate.

4. Can the Feynman rules be applied to all nonlinear sigma models?

Yes, the Feynman rules can be applied to any nonlinear sigma model, regardless of the number of fields or symmetries involved. However, the calculations may become more complicated for models with a large number of fields.

5. How do the Feynman rules differ from other methods of calculating interactions in nonlinear sigma models?

The Feynman rules differ from other methods, such as perturbative methods, in that they are based on the principles of quantum field theory and take into account all possible interactions between particles. This allows for a more comprehensive and accurate calculation of scattering amplitudes.

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