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Quantization of enlarged Bianchi I universe

2008/06/15 by Shintaro Sawayama, Sawayama, Shintaro
Physics and Astronomy · #Astronomy and Astrophysical Research #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #High Energy Physics - Theory (hep-th) #gr-qc #hep-th

paper · pdf · doi:10.48550/arxiv.0806.2420

5 pages, no figures

openalex publication_date 2008/06/15 · arxiv created 2008/11/28 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We can solve the Wheeler-DeWitt equation of the enlarged Bianchi I as inhomogeneous type universe with static restriction which had been derived by previous paper. We consider the commutation relation between the static restriction and the Hamiltonian constraint. And we can simplify the usual 3+1 Hamiltonian constraint of the enlarged Biancki I type universe, and we finally show the state's form is the exponential. And we find that the states of the quantum gravity are entangled. Our paper based on the previous work of ours that we call up-to-down method which was aimed to simplify the Wheeler-DeWitt equation.

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