Residual Representations of Spacetime
| dc.creator | Saller, Heinrich | |
| dc.date | 2000-10-09 | |
| dc.date.accessioned | 2026-07-07T04:10:40Z | |
| dc.date.available | 2026-07-07T04:10:40Z | |
| dc.description | Spacetime is modelled by binary relations - by the classes of the automorphisms $\GL(\C^2)$ of a complex 2-dimensional vector space with respect to the definite unitary subgroup $\U(2)$. In extension of Feynman propagators for particle quantum fields representing only the tangent spacetime structure, global spacetime representations are given, formulated as residues using energy-momentum distributions with the invariants as singularities. The associatated quantum fields are characterized by two invariant masses - for time and position - supplementing the one mass for the definite unitary particle sector with another mass for the indefinite unitary interaction sector without asymptotic particle interpretation. | |
| dc.description | 30 pages, latex, macros included | |
| dc.identifier | https://arxiv.org/abs/hep-th/0010057 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0010057 | |
| dc.identifier | Int.J.Theor.Phys. 40 (2001) 1209-1248 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/50293 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Residual Representations of Spacetime | |
| dc.type | text |