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Back to Basics?... or How can supersymmetry be used in simple quantum cosmological model

1995/05/02 by Paulo Vargas Moniz, P. V. Moniz, Moniz, P. V.
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Noncommutative and Quantum Gravity Theories #gr-qc

paper · pdf · doi:10.48550/arxiv.gr-qc/9505002

6 pages; Communication presented at the First Mexican School in Gravitation and Mathematical Physics, Guanajuato, Mexico, December 12-16, 1994; TeX macro for table at the end of file

arxiv created 1995/05/02 · openalex publication_date 1995/05/02 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

The general theory of N=1 supergravity with supermatter is applied to a Bianchi type IX diagonal model. The supermatter is constituted by a complex scalar field and its spin-1\over 2 fermionic partners. The Lorentz invariant Ansatz for the wave function of the universe, Ψ, is taken to be as simple as possible in order to obtain \it new solutions. The wave function has a simple form when the potential energy term is set to zero. However, neither the wormhole or the Hartle-Hawking state could be found. The Ansatz for Ψ used in this paper is constrasted with the more general framework of R. Graham and A. Csordás.

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