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dc.contributor.authorHaro Cases, Jaume
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Matemàtiques
dc.date.accessioned2016-05-05T10:19:37Z
dc.date.available2016-05-05T10:19:37Z
dc.date.issued2014-07-08
dc.identifier.citationHaro, J. How can holonomy corrections be introduced in f(R) gravity?. "Europhysics letters", 08 Juliol 2014, vol. 107, núm. 2.
dc.identifier.issn0295-5075
dc.identifier.urihttp://hdl.handle.net/2117/86623
dc.description.abstractWe study the introduction of holonomy corrections in f(R) gravity. We will show that there are infinitely many ways, as many as canonical transformations, to introduce this kind of corrections, depending on the canonical variables (two coordinates and its conjugate momenta) used to obtain the Hamiltonian. In each case, these corrections lead, at effective level, to different modified holonomy-corrected Friedmann equations in f(R) gravity, which are in practice analytically unworkable, i.e. only numerical analysis can be used to understand its dynamics. In fact, there are infinitely many quantum theories, as many as canonical transformations, leading to different quantum cosmologies. Then, the problem is to know which of these quantum theories apply correctly to our Universe. We do not have an answer to this problem, and we could only give the following argument in favour of one preferred set of variables: the one that conformally maps f(R) to Einstein gravity, because for these variables the Hamiltonian of the system has the same form as in standard Loop Quantum Cosmology, which provides a map between the dynamics obtained in holonomy-corrected f(R) gravity and the one of standard Loop Quantum Cosmology. © CopyrightEPLA, 2014.
dc.language.isoeng
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subjectÀrees temàtiques de la UPC::Matemàtiques i estadística
dc.subject.lcshCosmology
dc.subject.otherGravitation and cosmology
dc.subject.otherAstrophysics and astroparticles
dc.titleHow can holonomy corrections be introduced in f(R) gravity?
dc.typeArticle
dc.subject.lemacCosmologia
dc.contributor.groupUniversitat Politècnica de Catalunya. EDP - Equacions en Derivades Parcials i Aplicacions
dc.identifier.doi10.1209/0295-5075/107/29001
dc.description.peerreviewedPeer Reviewed
dc.relation.publisherversionhttp://iopscience.iop.org/0295-5075/107/2/29001/
dc.rights.accessOpen Access
local.identifier.drac15206548
dc.description.versionPostprint (published version)
local.citation.authorHaro, J.
local.citation.publicationNameEurophysics letters
local.citation.volume107
local.citation.number2


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