Feynman rules for nonlinear sigma models

Click For Summary
SUMMARY

Nonlinear sigma models are field theories where fields take values in nontrivial manifolds, leading to constraints in the Lagrangian. The Faddeev-Popov procedure is essential for quantizing these constrained systems, allowing the conversion of functional integrals over constrained fields to unconstrained fields, including auxiliary fields. In the context of the CP(N-1) model, the introduction of auxiliary fields, specifically a vector field Aμ and a scalar field σ, allows for the rewriting of the Lagrangian and facilitates the integration of n, resulting in an effective action dependent on these auxiliary fields. This approach reveals that interactions among n generate a gauge field Aμ, leading to confinement of the original degrees of freedom.

PREREQUISITES
  • Understanding of nonlinear sigma models
  • Faddeev-Popov quantization procedure
  • Familiarity with the CP(N-1) model
  • Knowledge of auxiliary fields in quantum field theory
NEXT STEPS
  • Study the Faddeev-Popov procedure in detail
  • Explore the implications of auxiliary fields in quantum field theories
  • Research the CP(N-1) model and its applications in 2D
  • Examine the role of gauge fields in nonlinear sigma models
USEFUL FOR

The discussion is beneficial for theoretical physicists, particularly those specializing in quantum field theory, as well as researchers working on nonlinear sigma models and their quantization methods.

hyperkahler
Messages
2
Reaction score
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 CP(N-1) model:

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

where n is a N-component vector of complex scalars with the constrained n^\dagger n=1. My problem is that this constraint leads to a new lagrangian term \lambda(n^\dagger n-1) (introducing an auxiliary field \lambda 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?
 
Physics news on Phys.org
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.
 

Similar threads

  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 134 ·
5
Replies
134
Views
12K
  • · Replies 24 ·
Replies
24
Views
3K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 20 ·
Replies
20
Views
4K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 7 ·
Replies
7
Views
5K
  • · Replies 3 ·
Replies
3
Views
5K
Replies
6
Views
3K