paper

Quantum Discrete Levels of the Universe from the Early Trans-Planckian Vacuum to the Late Dark Energy

arXiv:2004.09257 · doi:10.1103/PhysRevD.104.123517

Abstract

The standard model of the universe is further completed back in time before inflation in agreement with observations, classical-quantum gravity duality and quantum space-time. Quantum vacuum energy bends the space-time and produces a constant curvature de Sitter background. We link de Sitter universe and the cosmological constant to the (classical and quantum) harmonic oscillator. Quantum discrete cosmological levels are found: size, time, vacuum energy, Hubble constant and gravitational (Gibbons-Hawking) entropy from the very early trans-planckian vacuum to the classical today vacuum energy. For each level , the two: post and pre (trans)-planckian phases are covered: In the post-planckian universe, the levels (in planck units) are: Hubble constant , vacuum energy , entropy . As increases, radius, mass and increase, and decrease and {\it consistently} the universe {\it classicalizes}. In the pre-planckian (trans-planckian) phase, the quantum levels are: , denoting quantum. The -levels cover {\it all} scales from the far past highest excited trans-planckian level with finite curvature, and minimum entropy , decreases till the planck level and enters the post-planckian phase e.g: with the most classical value , , . We implement the Snyder-Yang algebra in this context yielding a consistent group-theory realization of quantum discrete de Sitter space-time, classical-quantum gravity duality symmetry and a clarifying unifying picture.(Abridged)

Published version in Phys Rev D, 54 pages, 1 figure, new material. arXiv admin note: text overlap with arXiv:1912.06655

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