Snyder's Model -- de Sitter Special Relativity Duality and de Sitter Gravity

dc.creatorGuo, Han-Ying
dc.creatorHuang, Chao-Guang
dc.creatorTian, Yu
dc.creatorWu, Hong-Tu
dc.creatorXu, Zhan
dc.creatorZhou, Bin
dc.date2007-03-14
dc.date2007-08-14
dc.date.accessioned2026-07-07T11:21:53Z
dc.date.available2026-07-07T11:21:53Z
dc.descriptionBetween Snyder's quantized space-time model in de Sitter space of momenta and the \dS special relativity on \dS-spacetime of radius $R$ with Beltrami coordinates, there is a one-to-one dual correspondence supported by a minimum uncertainty-like argument. Together with Planck length $\ell_P$, $R\simeq (3/Λ)^{1/2}$ should be a fundamental constant. They lead to a dimensionless constant $g{\sim\ell_PR^{-1}}=(G\hbar c^{-3}Λ/3)^{1/2}\sim 10^{-61}$. These indicate that physics at these two scales should be dual to each other and there is in-between gravity of local \dS-invariance characterized by $g$. A simple model of \dS-gravity with a gauge-like action on umbilical manifolds may show these characters. It can pass the observation tests and support the duality.
dc.description32 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0703078
dc.identifierhttp://arxiv.org/abs/gr-qc/0703078
dc.identifierClass.Quant.Grav.24:4009-4036,2007
dc.identifierdoi:10.1088/0264-9381/24/16/004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194395
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSnyder's Model -- de Sitter Special Relativity Duality and de Sitter Gravity
dc.typetext

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