Dynamical Symmetry Breaking in Einstein Universe
| dc.creator | Ishikawa, K. | |
| dc.creator | Inagaki, T. | |
| dc.creator | Muta, T. | |
| dc.date | 1995-12-28 | |
| dc.date.accessioned | 2026-07-07T04:21:47Z | |
| dc.date.available | 2026-07-07T04:21:47Z | |
| dc.description | We investigate four-fermion interactions with $N$-component fermion in Einstein universe for arbitrary space-time dimensions ($2 \leq D<4$). It is found that the effective potential for composite operator $\overlineψψ$ is calculable in the leading order of the $1/N$ expansion. The resulting effective potential is analyzed by varying the curvature of the space-time and is found to exhibit the symmetry restoration through the second-order phase transition. The critical curvature at which the dynamical fermion mass disappears is analytically calculated. | |
| dc.description | 13 pages, uses LaTeX, here.sty, epic.sty, eepic.sty | |
| dc.identifier | https://arxiv.org/abs/hep-th/9512202 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9512202 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/54461 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Dynamical Symmetry Breaking in Einstein Universe | |
| dc.type | text |