Quantcast
  • Register
PhysicsOverflow is a next-generation academic platform for physicists and astronomers, including a community peer review system and a postgraduate-level discussion forum analogous to MathOverflow.

Welcome to PhysicsOverflow! PhysicsOverflow is an open platform for community peer review and graduate-level Physics discussion.

Please help promote PhysicsOverflow ads elsewhere if you like it.

News

PO is now at the Physics Department of Bielefeld University!

New printer friendly PO pages!

Migration to Bielefeld University was successful!

Please vote for this year's PhysicsOverflow ads!

Please do help out in categorising submissions. Submit a paper to PhysicsOverflow!

... see more

Tools for paper authors

Submit paper
Claim Paper Authorship

Tools for SE users

Search User
Reclaim SE Account
Request Account Merger
Nativise imported posts
Claim post (deleted users)
Import SE post

Users whose questions have been imported from Physics Stack Exchange, Theoretical Physics Stack Exchange, or any other Stack Exchange site are kindly requested to reclaim their account and not to register as a new user.

Public \(\beta\) tools

Report a bug with a feature
Request a new functionality
404 page design
Send feedback

Attributions

(propose a free ad)

Site Statistics

205 submissions , 163 unreviewed
5,082 questions , 2,232 unanswered
5,353 answers , 22,789 comments
1,470 users with positive rep
820 active unimported users
More ...

  How do WZW coset models contain perturbations?

+ 5 like - 0 dislike
864 views

I've been studying the coset construction. As far as I understand it, the Sugawara energy momentum tensor is a way of embedding the Virasoro algebra inside the Lie algebra of your original WZW model. The nice thing is that the weight modules match (descending weights in the Virasoro rep match descendants of primary fields in the cft).

Different choices for the original Lie algebra lead to different CFTs. Most notably, taking the diagonal coset of the affine extension of su(2): $$\frac{\widehat{\mathfrak{su}}(2)_k\oplus \widehat{\mathfrak{su}}(2)_1}{\widehat{\mathfrak{su}}(2)_{k+1}}$$

leads to the set of minimal models. However, I've also been reading, for example in di Francesco (the big yellow book), that some of these coset WZW models correspond to perturbed CFTs. For example, diagonal $\widehat{\mathfrak{su}}(2)_k$ and $\widehat{E_{(8)}}_k$ at k=1 lead to the Ising model perturbed with respectively energy density and an external magnetic field.

My confusion is the following: If these diagonal coset models lead to CFTs, how can they also describe perturbed theories? Does this perturbation not destroy conformal invariance? More concretely: When investigating the field content of the coset model by looking at the character decompositions, how do you find out what the perturbation is?


This post imported from StackExchange Physics at 2017-10-27 21:14 (UTC), posted by SE-user Abel Jansma

asked Sep 18, 2017 in Theoretical Physics by Abel Jansma (25 points) [ revision history ]
edited Oct 27, 2017 by Dilaton

Maybe "perturbed" is the same thing as "interacting"?

Your answer

Please use answers only to (at least partly) answer questions. To comment, discuss, or ask for clarification, leave a comment instead.
To mask links under text, please type your text, highlight it, and click the "link" button. You can then enter your link URL.
Please consult the FAQ for as to how to format your post.
This is the answer box; if you want to write a comment instead, please use the 'add comment' button.
Live preview (may slow down editor)   Preview
Your name to display (optional):
Privacy: Your email address will only be used for sending these notifications.
Anti-spam verification:
If you are a human please identify the position of the character covered by the symbol $\varnothing$ in the following word:
p$\hbar$ysicsOverfl$\varnothing$w
Then drag the red bullet below over the corresponding character of our banner. When you drop it there, the bullet changes to green (on slow internet connections after a few seconds).
Please complete the anti-spam verification




user contributions licensed under cc by-sa 3.0 with attribution required

Your rights
...