Adeegso tilmaantan si aad u carrabbaabdo ama ugu samayso link qoraalkan http://hdl.handle.net/2307/585
Bed DCQiimoLuqad
dc.contributor.advisorRagnisco, Orlando-
dc.contributor.authorMagliaro, Elena-
dc.contributor.otherRovelli, Carlo-
dc.date.accessioned2011-08-05T11:52:41Z-
dc.date.available2011-08-05T11:52:41Z-
dc.date.issued2009-01-12-
dc.identifier.urihttp://hdl.handle.net/2307/585-
dc.description.abstractIn this doctoral thesis I developed techniques for the study of the low energy limit in Loop Quantum Gravity. Loop Quantum Gravity is a strong candidate theory for the non-perturbative quantization of the gravitational field. Though is unlikely that an experimental verification could be feasible in the next future, one can at least try to recover the correct semiclassical limit of the theory. First of all, the leading order of the 2-point function computed in LQG should reproduce the Newtonian potential in the large distance regime; more in general, the n-point functions of LQG should match with the n-point functions computed in conventional quantum field theory of gravitons. An origianal contribution to the calculation of the graviton propagator in LQG is presented. A second approach to the semiclassical limit is introduced for the first time in this thesis, and it is based on the coherent propagation of semiclassical wavepackets. Both approaches to the analysis of the dynamical sector of LQG are covered extensively.it_IT
dc.language.isoenit_IT
dc.publisherUniversità degli studi Roma Treit_IT
dc.titleLow energy limit in Loop Quantum Gravityit_IT
dc.typeDoctoral Thesisit_IT
dc.subject.miurSettori Disciplinari MIUR::Scienze fisiche::FISICA TEORICA, MODELLI E METODI MATEMATICIit_IT
dc.subject.miurScienze fisiche-
dc.subject.anagraferoma3Scienze fisicheit_IT
local.testtest-
dc.description.romatrecurrentDipartimento di Fisica 'Edoardo Amaldi'*
item.fulltextWith Fulltext-
item.grantfulltextopen-
item.languageiso639-1other-
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