2007/05/07 by Otto C. W. Kong, Kong, Otto C. W.
Physics and Astronomy · #Black Holes and Theoretical Physics #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #High Energy Physics - Theory (hep-th) #Noncommutative and Quantum Gravity Theories #Particle physics theoretical and experimental studies #gr-qc #hep-th
paper · pdf · doi:10.48550/arxiv.0705.0845
10 pages of revtex, no figure;a largely rewritten presentation of the same results
openalex publication_date 2007/05/07 · arxiv created 2008/01/25 · arxiv updated 2011/11/09 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Quantum relativity as a generalized, or rather deformed, version of Einstein relativity with a linear realization on a classical six-geometry beyond the familiar setting of space-time offer a new framework to think about the quantum space-time structure. The formulation requires two deformations to be implemented through imposing two fundamental invariants. We take them to be the independent Planck mass and Planck length. Together, they gives the quantum ℏ. The scheme leads to \small \boldmath\protect SO(2,4) as the relativity symmetry. The quantum world has an AdS5 `classical' geometry, which is parallel to the "conformal universe", but not scale invariant.