Exponentially Small Supersymmetry Breaking from Extra Dimensions
| dc.creator | Arkani-Hamed, Nima | |
| dc.creator | Hall, Lawrence | |
| dc.creator | Smith, David | |
| dc.creator | Weiner, Neal | |
| dc.date | 1999-11-22 | |
| dc.date | 1999-12-18 | |
| dc.date.accessioned | 2026-07-07T11:47:54Z | |
| dc.date.available | 2026-07-07T11:47:54Z | |
| dc.description | The supersymmetric ``shining'' of free massive chiral superfields in extra dimensions from a distant source brane can trigger exponentially small supersymmetry breaking on our brane of order e^{-2 pi R}, where R is the radius of the extra dimensions. This supersymmetry breaking can be transmitted to the superpartners in a number of ways, for instance by gravity or via the standard model gauge interactions. The radius R can easily be stabilized at a size O(10) larger that the fundamental scale. The models are extremely simple, relying only on free, classical bulk dynamics to solve the hierarchy problem. | |
| dc.description | RevTex, 1 figure. Comment on mu problem added | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9911421 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9911421 | |
| dc.identifier | Phys.Rev.D63:056003,2001 | |
| dc.identifier | doi:10.1103/PhysRevD.63.056003 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/202739 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Exponentially Small Supersymmetry Breaking from Extra Dimensions | |
| dc.type | text |