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dc.contributor.authorBodmann, Benno August Ludwigpt_BR
dc.contributor.authorVasconcellos, Cesar Augusto Zenpt_BR
dc.contributor.authorHess, Peter Ottopt_BR
dc.contributor.authorPacheco, Jose Antonio de Freitaspt_BR
dc.contributor.authorHadjimichef, Dimiterpt_BR
dc.contributor.authorRazeira, Moisespt_BR
dc.contributor.authorDegrazia, Gervasio Annespt_BR
dc.date.accessioned2024-09-03T06:41:50Zpt_BR
dc.date.issued2023pt_BR
dc.identifier.issn2218-1997pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/278377pt_BR
dc.description.abstractIn this contribution to the Festschrift for Prof. Remo Ruffini, we investigate a formulation of quantum gravity using the Hořava–Lifshitz theory of gravity, which is General Relativity augmented by counter-terms to render the theory regularized. We are then led to the Wheeler–DeWitt (WDW) equation combined with the classical concepts of the branch-cut gravitation, which contemplates as a new scenario for the origin of the Universe, a smooth transition region between the contraction and expansion phases. Through the introduction of an energy-dependent effective potential, which describes the space-time curvature associated with the embedding geometry and its coupling with the cosmological constant and matter fields, solutions of the WDW equation for the wave function of the Universe are obtained. The Lagrangian density is quantized through the standard procedure of raising the Hamiltonian, the helix-like complex scale factor of branched gravitation as well as the corresponding conjugate momentum to the category of quantum operators. Ambiguities in the ordering of the quantum operators are overcome with the introduction of a set of ordering factors 𝛼 , whose values are restricted, to make contact with similar approaches, to the integers 𝛼=[0,1,2], allowing this way a broader class of solutions for the wave function of the Universe. In addition to a branched universe filled with underlying background vacuum energy, primordial matter and radiation, in order to connect with standard model calculations, we additionally supplement this formulation with baryon matter, dark matter and quintessence contributions. Finally, the boundary conditions for the wave function of the Universe are imposed by assuming the Bekenstein criterion. Our results indicate the consistency of a topological quantum leap, or alternatively a quantum tunneling, for the transition region of the early Universe in contrast to the classic branched cosmology view of a smooth transition.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofUniverse. Basel. Vol. 9, no. 6 (June 2023), 278, 16 p.pt_BR
dc.rightsOpen Accessen
dc.subjectBranch-cut cosmologyen
dc.subjectGravidade quânticapt_BR
dc.subjectWheeler–DeWitt equationen
dc.subjectEspaço e tempopt_BR
dc.subjectQuantum gravityen
dc.subjectCosmologiapt_BR
dc.titleA Wheeler–DeWitt quantum approach to the branch-cut gravitation with ordering parameterspt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb001196992pt_BR
dc.type.originEstrangeiropt_BR


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