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Solvable loop quantum cosmology: domain of the volume observable and semiclassical states

dc.contributor.authorMartín Benito, Mercedes
dc.contributor.authorNeves, Rita B.
dc.date.accessioned2025-01-08T18:02:00Z
dc.date.available2025-01-08T18:02:00Z
dc.date.issued2019-02-19
dc.description.abstractThe dynamics of a flat Friedmann-Lemaître-Robertson-Walker model minimally coupled to a massless scalar field has been intensively studied in the context of loop quantum cosmology (LQC). This model admits an appropriate solvable representation, named sLQC. The form of the domain of the volume, the main observable to track the quantum evolution, is not straightforward in this solvable representation, and its explicit construction has been overlooked so far. In this work we find the explicit form of physical states belonging to the domain of the volume in sLQC. Specifically, given a physical state in the 𝑣-representation where the volume acts diagonally, we derive its form in the representation employed in sLQC, making explicit the connection between both representations at the physical level. To this end, we resort to the Wheeler-De Witt (WDW) approach, which shares the physical Hilbert space with sLQC when cast in an analog solvable representation, while being analytically solvable as well in the 𝑣-representation. Then the domain of the volume for the WDW approach provides that for sLQC. Furthermore, we address the question of semiclassicality in sLQC.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.facultyInstituto de Física de Partículas y del Cosmos (IPARCOS)
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Economia y Competitividad (España)
dc.description.sponsorshipAgencia Estatal de Investigación (España)
dc.description.sponsorshipFundação para a Ciência e a Tecnologia (Portugal)
dc.description.statuspub
dc.identifier.citationMartín-Benito, M., & Neves, R. B. (2019). Solvable Loop Quantum Cosmology: domain of the volume observable and semiclassical states. Physical Review D, 99(4), 043525.
dc.identifier.doi10.1103/physrevd.99.043525
dc.identifier.essn2470-0029
dc.identifier.issn2470-0010
dc.identifier.officialurlhttps://doi.org/10.1103/PhysRevD.99.043525
dc.identifier.relatedurlhttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.99.043525
dc.identifier.urihttps://hdl.handle.net/20.500.14352/113350
dc.issue.number4
dc.journal.titlePhysical Review D
dc.language.isoeng
dc.page.final043525-13
dc.page.initial043525-01
dc.publisherAmerican Physical Society
dc.relation.projectIDinfo:eu-repo/grantAgreement/MINECO//FIS2014-54800-C2-2-P/ES/GRAVEDAD Y UNIVERSO CUANTICO: COSMOLOGIA DE LAZOS, AGUJEROS NEGROS Y FRACTALES/
dc.relation.projectIDinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/FIS2017-86497-C2-2-P/ES/UNIVERSO Y VACIO CUANTICOS: GRAVEDADES MULTIESCALA, COSMOLOGIA CUANTICA DE LAZOS Y AGUJEROS NEGROS/
dc.relation.projectIDPTDC/FIS-OUT/29048/2017
dc.rights.accessRightsopen access
dc.subject.cdu530.145
dc.subject.cdu51
dc.subject.keywordQuantum Cosmology
dc.subject.ucmTeoría de los quanta
dc.subject.unesco2212 Física Teórica
dc.titleSolvable loop quantum cosmology: domain of the volume observable and semiclassical states
dc.typejournal article
dc.type.hasVersionAO
dc.volume.number99
dspace.entity.typePublication
relation.isAuthorOfPublicatione4763414-91cd-42f1-b41a-76fc60c6f215
relation.isAuthorOfPublication.latestForDiscoverye4763414-91cd-42f1-b41a-76fc60c6f215

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