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dc.contributor.authorBodmann, Benno August Ludwigpt_BR
dc.contributor.authorHadjimichef, Dimiterpt_BR
dc.contributor.authorHess, Peter Ottopt_BR
dc.contributor.authorPacheco, Jose Antonio de Freitaspt_BR
dc.contributor.authorWeber, Fridolinpt_BR
dc.contributor.authorRazeira, Moisespt_BR
dc.contributor.authorDegrazia, Gervasio Annespt_BR
dc.contributor.authorMarzola, Marcelo Netzpt_BR
dc.contributor.authorVasconcellos, Cesar Augusto Zenpt_BR
dc.date.accessioned2024-09-06T06:38:43Zpt_BR
dc.date.issued2023pt_BR
dc.identifier.issn2218-1997pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/278486pt_BR
dc.description.abstractIn this contribution, motivated by the quest to understand cosmic acceleration, based on the theory of Hoˇrava–Lifshitz and on the branch-cut gravitation, we investigate the effects of non-commutativity of a mini-superspace of variables obeying the Poisson algebra on the structure of the branch-cut scale factor and on the acceleration of the Universe. We follow the guiding lines of a previous approach, which we complement to allow a symmetrical treatment of the Poisson algebraic variables and eliminate ambiguities in the ordering of quantum operators. On this line of investigation, we propose a phase-space transformation that generates a super-Hamiltonian, expressed in terms of new variables, which describes the behavior of a Wheeler–DeWitt wave function of the Universe within a non-commutative algebraic quantum gravity formulation. The formal structure of the super-Hamiltonian allows us to identify one of the new variables with a modified branch-cut quantum scale factor, which incorporates, as a result of the imposed variable transformations, in an underlying way, elements of the non-commutative algebra. Due to its structural character, this algebraic structure allows the identification of the other variable as the dual quantum counterpart of the modified branch-cut scale factor, with both quantities scanning reciprocal spaces. Using the iterative Range–Kutta–Fehlberg numerical analysis for solving differential equations, without resorting to computational approximations, we obtained numerical solutions, with the boundary conditions of the wave function of the Universe based on the Bekenstein criterion, which provides an upper limit for entropy. Our results indicate the acceleration of the early Universe in the context of the non-commutative branch-cut gravity formulation. These results have implications when confronted with information theory; so to accommodate gravitational effects close to the Planck scale, a formulation à la Heisenberg’s Generalized Uncertainty Principle in Quantum Mechanics involving the energy and entropy of the primordial Universe is proposed.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofUniverse. Basel. Vol. 9, no. 10 (Oct. 2023), 428, 24 p.pt_BR
dc.rightsOpen Accessen
dc.subjectBranch-cut cosmologyen
dc.subjectCosmologiapt_BR
dc.subjectEquação de Wheeler–DeWittpt_BR
dc.subjectWheeler–DeWitt equationen
dc.subjectGravidade quânticapt_BR
dc.subjectNon-commutative quantum gravityen
dc.titleA Wheeler–DeWitt non-commutative quantum approach to the branch-cut gravitypt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb001199576pt_BR
dc.type.originEstrangeiropt_BR


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