Very Special Relativity in Curved Space-Times
| dc.creator | Mueck, Wolfgang | |
| dc.date | 2008-06-04 | |
| dc.date.accessioned | 2026-07-07T12:14:39Z | |
| dc.date.available | 2026-07-07T12:14:39Z | |
| dc.description | The generalization of Cohen and Glashow's Very Special Relativity to curved space-times is considered. Gauging the SIM(2) symmetry does not, in general, provide the coupling to the gravitational background. However, locally SIM(2) invariant Lagrangians can always be constructed. For space-times with SIM(2) holonomy, they describe chiral fermions propagating freely as massive particles. | |
| dc.description | 7 pages | |
| dc.identifier | https://arxiv.org/abs/0806.0737 | |
| dc.identifier | http://arxiv.org/abs/0806.0737 | |
| dc.identifier | Phys.Lett.B670:95-98,2008 | |
| dc.identifier | doi:10.1016/j.physletb.2008.10.028 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/211266 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Very Special Relativity in Curved Space-Times | |
| dc.type | text |