Twisted Covariance vs Weyl Quantisation
dc.contributor.area | Mathematics | en_US |
dc.contributor.author | Piacitelli, Gherardo | en_US |
dc.contributor.department | Mathematical Physics | en_US |
dc.date.accessioned | 2009-01-22T12:32:39Z | en_US |
dc.date.accessioned | 2011-09-07T20:21:21Z | |
dc.date.available | 2009-01-22T12:32:39Z | en_US |
dc.date.available | 2011-09-07T20:21:21Z | |
dc.date.issued | 2009-01-22T12:32:39Z | en_US |
dc.description.abstract | In this letter we wish to clarify in which sense the tensor nature of the commutation relations [x^mu,x^nu]=i theta ^{mu nu} underlying Minkowski spacetime quantisation cannot be suppressed even in the twisted approach to Lorentz covariance. We then address the vexata quaestio "why theta"? | en_US |
dc.format.extent | 135129 bytes | en_US |
dc.format.mimetype | application/pdf | en_US |
dc.identifier.uri | https://openscience.sissa.it/handle/1963/3451 | en_US |
dc.language.iso | en_US | en_US |
dc.relation.ispartofseries | SISSA;13/2009/FM | en_US |
dc.relation.ispartofseries | arXiv.org;0901.3109v1 | en_US |
dc.title | Twisted Covariance vs Weyl Quantisation | en_US |
dc.type | Preprint | en_US |