A relativistic variant of the Wigner function
| dc.creator | Morgan, Peter | |
| dc.date | 2003-04-28 | |
| dc.date | 2003-12-17 | |
| dc.date.accessioned | 2026-07-07T06:06:38Z | |
| dc.date.available | 2026-07-07T06:06:38Z | |
| dc.description | The conventional Wigner function is inappropriate in a quantum field theory setting because, as a quasiprobability density over phase space, it is not manifestly Lorentz covariant. A manifestly relativistic variant is constructed as a quasiprobability density over trajectories instead of over phase space. | |
| dc.description | v3: as accepted by Phys. Lett. A | |
| dc.identifier | https://arxiv.org/abs/quant-ph/0304171 | |
| dc.identifier | http://arxiv.org/abs/quant-ph/0304171 | |
| dc.identifier | Phys.Lett. A321 (2004) 216-224 | |
| dc.identifier | doi:10.1016/j.physleta.2003.12.029 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/91048 | |
| dc.subject | Quantum Physics | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | A relativistic variant of the Wigner function | |
| dc.type | text |