Non trivial spacetime effects in a supersymmetric model
| dc.creator | Oikonomou, V. K. | |
| dc.date | 2006-11-07 | |
| dc.date.accessioned | 2026-07-07T11:02:08Z | |
| dc.date.available | 2026-07-07T11:02:08Z | |
| dc.description | We study a ${N=1}$ supersymmetric model in a ${S}^{1}{\times R}^{3}$ spacetime. We find that by choosing appropriate boundary conditions for the contributing fields supersymmetry can be preserved. However if we add a hard supersymmetry breaking term, we observe that for small values of the length of the ${S}^{1}$ dimension, supersymmetry remains unbroken and breaks spontaneously when the length exceeds a critical value. The final picture resembles the first order phase transition picture. | |
| dc.description | 12 pages, 3 figures | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0611079 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0611079 | |
| dc.identifier | J.Phys.A40:9929,2007; J.Phys.A40:9929-9940,2007 | |
| dc.identifier | doi:10.1088/1751-8113/40/32/016 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/188157 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Non trivial spacetime effects in a supersymmetric model | |
| dc.type | text |