Back to Basics?... or How can supersymmetry be used in simple quantum cosmological model
| dc.creator | Moniz, P. V. | |
| dc.date | 1995-05-02 | |
| dc.date.accessioned | 2026-07-07T03:30:40Z | |
| dc.date.available | 2026-07-07T03:30:40Z | |
| dc.description | 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. | |
| dc.description | 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 | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9505002 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9505002 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/35600 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Back to Basics?... or How can supersymmetry be used in simple quantum cosmological model | |
| dc.type | text |