Kaluza -- Klein Quantum Cosmology with Primordial Negative Cosmological Constant

dc.creatorGuendelman, E. I.
dc.creatorKaganovich, A. B.
dc.date1994-08-25
dc.date.accessioned2026-07-07T03:30:25Z
dc.date.available2026-07-07T03:30:25Z
dc.descriptionIn many interesting models, including superstring theories, a negative vacuum energy is predicted. Although this effect is usually regarded as undesirable from a cosmological point of view, we show that this can be the basis for a new approach to the cosmology of the early Universe. In the framework of quantum cosmology (in higher dimensions) when we consider a negative cosmological constant and matter that could be dust or, alternatively, coherent excitations of a scalar field, the role of cosmic time can be understood. Then we can predict the existence of a ``quantum inflationary phase'' for some dimensions and a simultaneous ``quantum deflationary phase'' for the remaining dimensions. We discuss how it may be possible to exit from this inflation-compactification era to a phase with zero cosmological constant which allows a classical description at late times.
dc.description5 pages, Latex, BGU-94/17/August-PH
dc.identifierhttps://arxiv.org/abs/gr-qc/9408031
dc.identifierhttp://arxiv.org/abs/gr-qc/9408031
dc.identifierGrav.Cosmol. 1 (1995) 103-105
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35527
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleKaluza -- Klein Quantum Cosmology with Primordial Negative Cosmological Constant
dc.typetext

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