Large volume quantum correction in loop quantum cosmology: Graviton illusion?

dc.creatorHossain, Golam Mortuza
dc.date2005-04-25
dc.date.accessioned2026-07-07T03:29:40Z
dc.date.available2026-07-07T03:29:40Z
dc.descriptionThe leading quantum correction to Einstein-Hilbert Hamiltonian coming from large volume vacuum isotropic loop quantum cosmology, is independent of quantization ambiguity parameters. It is shown here that this correction can be viewed as finite volume gravitational Casimir energy due to one-loop `graviton' contributions. In vacuum case sub-leading quantum corrections and in non-vacuum case even leading quantum correction depend on ambiguity parameters. It may be recalled that these are in fact analogous features of perturbative quantum gravity where it is well-known that pure gravity (on-shell) is one-loop finite whereas higher-loops contributions are not even renormalizable. These features of the quantum corrections coming from non-perturbative quantization, sheds a new light on a major open issue; how to communicate between non-perturbative and perturbative approaches of quantum gravity.
dc.descriptionrevtex4, 4 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0504125
dc.identifierhttp://arxiv.org/abs/gr-qc/0504125
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35269
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleLarge volume quantum correction in loop quantum cosmology: Graviton illusion?
dc.typetext

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