Lobachevsky-Poincaré-Dirac Space and Quantum Nature of Internal Spacetime versus External Space and Time in Cosmology
ORAL
Abstract
Some implications of an invariant model of Boltzmann statistical mechanics to thermodynamics [1] and quantum nature of space and time are described. Kelvin absolute temperature is identified as Wien wavelength λwb of thermal oscillations (kTβ = kλwβ = mβ(vwβ)2 , vwβ = λwβνwβ) and applied to introduce internal measures of space and time called spacetime (λwβ-1, τwβ-1) and external measures of space and time (xβ = Nxλwβ-1, tβ = Ntτwβ-1). Because of its hyperbolic geometry, its discrete fabric, and its stochastic atomic motions, physical space is called Lobachevsky-Poincaré-Dirac-Space. When Casimir vacuum is identified as Planck compressible ether, Lorentz-FitzGerald contractions become causal, Pauli [2], in accordance with Poincaré-Lorentz dynamic as opposed to Einstein kinematic theory of relativity [3]. Mach, Lorentz, Michelson numbers (v/cm, v/ce, v/ck) lead to a unified description of supersonic, super-electronic, and superluminal flows involving (Mach, Lorentz, Poincaré-Minkowski) cones. The “time problem” of GTR and Gödel closed time-like world lines are also discussed.
1 Sohrab, S. H., ASME J. Energy Resoures Technology 138: 1-12 (2016).
2 Pauli, W., Theory of Relativity, Dover (1958).
3 Sohrab, S. H., Chaotic Modeling and Simulation (CMSIM) 3, 231-245 (2016).
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Presenters
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Siavash H Sohrab
Northwestern University
Authors
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Siavash H Sohrab
Northwestern University