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dc.contributor.authorRomano, Antonio Enea-
dc.contributor.authorChiang, Hsu-Wen-
dc.contributor.authorChen, Pisin-
dc.date.accessioned2024-06-18T19:53:21Z-
dc.date.available2024-06-18T19:53:21Z-
dc.date.issued2014-
dc.identifier.issn0264-9381-
dc.identifier.urihttps://hdl.handle.net/10495/40124-
dc.description.abstractABSTRACT: The luminosity distance can be used to determine the properties of large scale structure around the observer. To this purpose we develop a new inversion method to map luminosity distance to a LTB metric based on the use of the exact analytical solution for Einstein equations. The main advantages of this approach are an improved numerical accuracy and stability, an exact analytical setting of the initial conditions for the differential equations which need to be solved and the validity for any sign of the functions determining the LTB geometry. Given the fully analytical form of the differential equations, this method also simplifies the calculation of the red-shift expansion around the apparent horizon point where the numerical solution becomes unstable. We test the method by inverting the supernovae Ia luminosity distance function corresponding to the the best fit ΛCDM model. We find that only a limited range of initial conditions is compatible with observations, or a transition from red to blue shift can occur at relatively low redshift. Despite LTB solutions without a cosmological constant have been shown not to be compatible with all different set of available observational data, those studies normally fit data assuming a special functional ansatz for the inhomogeneity profile, which often depend only on few parameters. Inversion methods on the contrary are able to fully explore the freedom in fixing the functions which determine a LTB solution. For this reason this inversion method could be applied to explore more exhaustively the compatibility with observations. Another important possible application is not about LTB solutions as cosmological models, but rather as tools to study the effects on the observations made by a generic observer located in an inhomogeneous region of the Universe where a fully non perturbative treatment involving exact solutions of Einstein equations is required.spa
dc.format.extent20 páginasspa
dc.format.mimetypeapplication/pdfspa
dc.language.isoengspa
dc.publisherInstitute of Physicsspa
dc.type.hasversioninfo:eu-repo/semantics/acceptedVersionspa
dc.rightsinfo:eu-repo/semantics/openAccessspa
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/2.5/co/*
dc.subject.lcshDistancia de luminosidad-
dc.subject.lcshLuminosity distance-
dc.subject.lcshEstructura a gran escala (Astronomía)-
dc.subject.lcshLarge scale structure (Astronomy)-
dc.subject.lcshEcuaciones de campo de Einstein-
dc.subject.lcshEinstein field equations-
dc.titleA new method to determine large scale structure from the luminosity distancespa
dc.typeinfo:eu-repo/semantics/articlespa
dc.publisher.groupCOSMOGRAVspa
dc.identifier.doi10.1088/0264-9381/31/11/115008-
oaire.versionhttp://purl.org/coar/version/c_970fb48d4fbd8a85spa
dc.rights.accessrightshttp://purl.org/coar/access_right/c_abf2spa
dc.identifier.eissn1361-6382-
oaire.citationtitleClassical And Quantum Gravityspa
oaire.citationstartpage1spa
oaire.citationendpage20spa
oaire.citationvolume31spa
oaire.citationissue11spa
dc.rights.creativecommonshttps://creativecommons.org/licenses/by-nc-sa/4.0/spa
dc.publisher.placeBristol, Inglaterraspa
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1spa
dc.type.redcolhttps://purl.org/redcol/resource_type/ARTspa
dc.type.localArtículo de investigaciónspa
dc.subject.lcshurihttp://id.loc.gov/authorities/subjects/sh2003003637-
dc.subject.lcshurihttp://id.loc.gov/authorities/subjects/sh96004455-
dc.subject.lcshurihttp://id.loc.gov/authorities/subjects/sh85041416-
dc.description.researchgroupidCOL0147829spa
dc.relation.ispartofjournalabbrevClass. Quantum Gravity.spa
Aparece en las colecciones: Artículos de Revista en Ciencias Exactas y Naturales

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