BRST cohomology of Yang-Mills gauge fields in the presence of gravity in Ashtekar variables
| dc.creator | Moritsch, O. | |
| dc.creator | Schweda, M. | |
| dc.creator | Sommer, T. | |
| dc.creator | Tataru, L. | |
| dc.creator | Zerrouki, H. | |
| dc.date | 1994-09-14 | |
| dc.date.accessioned | 2026-07-07T04:20:31Z | |
| dc.date.available | 2026-07-07T04:20:31Z | |
| dc.description | The BRST transformations for the Yang-Mills gauge fields in the presence of gravity described by Ashtekar variables are obtained by using the so-called Maurer-Cartan horizontality conditions. The BRST cohomology group expressed by the Wess-Zumino consistency condition is solved with the help of an operator $δ$ introduced by S.P. Sorella which in our case has a very simple form and generates, together with the differential $d$ and the BRST operator $s$, a simpler algebra than in the pure Yang-Mills theory. In this way we shall find the Yang-Mills Lagrangians, the Chern-Simons terms and the gauge anomalies. | |
| dc.description | 20 pages, report REF.TUW 94-17 | |
| dc.identifier | https://arxiv.org/abs/hep-th/9409081 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9409081 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/53975 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | BRST cohomology of Yang-Mills gauge fields in the presence of gravity in Ashtekar variables | |
| dc.type | text |