Abstract

A class of two-dimensional sigma models interpolating between $CP^1$ and the $SU(2)$ principal chiral model is discussed. We add the Wess-Zumino-Novikov-Witten term and examine the renormalization group flow of the two coupling constants which characterize the model under consideration. The model flows to the $SU(2)$ WZNW conformal field theory in the IR. There is an ordinary phase in which the model flows from the asymptotically free $CP^1$ model coupled to an extra massless degree of freedom in the UV. At higher loop order we discover that there is also a phase in which the model can flow from non-trivial fixed points in the UV. A non-perturbative confirmation of these extra fixed points would be desirable.

Highlights

  • Nonlinear sigma models are often used as toy models in high energy physics to illuminate aspects of more realistic theories like QCD

  • For intermediate values of κ, the target space is a “squashed sphere” that is topologically equivalent to S2N−1, but which has a deformed metric along the Uð1Þ fibers of the fiber bundle defined by the natural map from S2N−1 → CPN−1

  • The only finite action field configurations are those which have a unique limit as the spacetime argument goes to infinity, and these field configurations map out a two-dimensional surface in the squashed sphere target space homeomorphic to S3

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Summary

INTRODUCTION

Nonlinear sigma models are often used as toy models in high energy physics to illuminate aspects of more realistic theories like QCD (see, e.g., [1]). A later rediscovery of the integrability [15] involves modifying the SUð2Þ current by a topological current so as to preserve the flatness condition [16] This result was extended to the squashed sphere with a WZNW term, as we consider here, and the RG flow was calculated to one loop [17,18]. Metsaev and Tseytlin [26] pointed out that the β functions in such theories depend on a renormalization scheme choice starting with two-loop order This generally speaking applies to our model as well as to the generic sigma models with metric gab and two-form gauge field hab, see Sec. II C.

INTRODUCING THE WZNW TERM
Adding a WZNW term
Renormalizing WZNW models
RG FLOW OF THE SQUASHED SPHERE WITH WZNW TERM
An exact RG trajectory
Additional fixed points
OF RESULTS
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