Tomographic Representation of Minisuperspace Quantum Cosmology and Noether Symmetries

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dc.creatorCapozziello, S.
dc.creatorMan'ko, V. I.
dc.creatorMarmo, G.
dc.creatorStornaiolo, C.
dc.date2007-06-20
dc.date2008-04-02
dc.date.accessioned2026-07-07T12:13:34Z
dc.date.available2026-07-07T12:13:34Z
dc.descriptionThe probability representation, in which cosmological quantum states are described by a standard positive probability distribution, is constructed for minisuperspace models selected by Noether symmetries. In such a case, the tomographic probability distribution provides the classical evolution for the models and can be considered an approach to select "observable" universes. Some specific examples, derived from Extended Theories of Gravity, are worked out. We discuss also how to connect tomograms, symmetries and cosmological parameters.
dc.description15 pages
dc.identifierhttps://arxiv.org/abs/0706.3018
dc.identifierhttp://arxiv.org/abs/0706.3018
dc.identifierGen.Rel.Grav.40:2627-2647,2008
dc.identifierdoi:10.1007/s10714-008-0643-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/210894
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleTomographic Representation of Minisuperspace Quantum Cosmology and Noether Symmetries
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