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- Q7923100 subject Q6617097.
- Q7923100 abstract "Ignoring gravity, experimental bounds seem to suggest that special relativity with its Lorentz symmetry and Poincaré symmetry describes spacetime. Surprisingly, Cohen and Glashow have demonstrated that a small subgroup of the Lorentz group is sufficient to explain all the current bounds.The minimal subgroup in question can be described as follows: The stabilizer of a null vector is the special Euclidean group SE(2), which contains T(2) as the subgroup of parabolic transformations. This T(2), when extended to include either parity or time reversal (i.e. subgroups of the orthochronous and time-reversal respectively), is sufficient to give us all the standard predictions. Their new symmetry is called Very Special Relativity (VSR).".
- Q7923100 wikiPageWikiLink Q1066449.
- Q7923100 wikiPageWikiLink Q1093427.
- Q7923100 wikiPageWikiLink Q11412.
- Q7923100 wikiPageWikiLink Q11455.
- Q7923100 wikiPageWikiLink Q1334417.
- Q7923100 wikiPageWikiLink Q141160.
- Q7923100 wikiPageWikiLink Q142270.
- Q7923100 wikiPageWikiLink Q288465.
- Q7923100 wikiPageWikiLink Q466109.
- Q7923100 wikiPageWikiLink Q488630.
- Q7923100 wikiPageWikiLink Q6617097.
- Q7923100 wikiPageWikiLink Q852195.
- Q7923100 comment "Ignoring gravity, experimental bounds seem to suggest that special relativity with its Lorentz symmetry and Poincaré symmetry describes spacetime. Surprisingly, Cohen and Glashow have demonstrated that a small subgroup of the Lorentz group is sufficient to explain all the current bounds.The minimal subgroup in question can be described as follows: The stabilizer of a null vector is the special Euclidean group SE(2), which contains T(2) as the subgroup of parabolic transformations.".
- Q7923100 label "Very special relativity".