The Classification of SU(3) Modular Invariants Revisited
| dc.creator | Gannon, Terry | |
| dc.date | 1994-04-29 | |
| dc.date.accessioned | 2026-07-07T04:20:11Z | |
| dc.date.available | 2026-07-07T04:20:11Z | |
| dc.description | The SU(3) modular invariant partition functions were first completely classified in Ref.\ \SU. The purpose of these notes is four-fold: \item{(i)} Here we accomplish the SU(3) classification using only the most basic facts: modular invariance; $M_{\laμ}\in{\bf Z}_{\ge}$; and $M_{00}=1$. In \SU{} we made use of less elementary results from Moore-Seiberg, in addition to these 3 basic facts. \item{(ii)} Ref.\ \SU{} was completed well over a year ago. Since then I have found a number of significant simplifications to the general argument. They are all included here. \item{(iii)} A number of people have complained that some of the arguments in \SU{} were hard to follow. I have tried here to be as explicit and as clear as possible. \item{(iv)} Hidden in \SU{} were a number of smaller results which should be of independent value. These are explicitly mentioned here. | |
| dc.description | 33 pp (plain tex) | |
| dc.identifier | https://arxiv.org/abs/hep-th/9404185 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9404185 | |
| dc.identifier | Annales Poincare Phys.Theor. 65 (1996) 15-56 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/53861 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | The Classification of SU(3) Modular Invariants Revisited | |
| dc.type | text |