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Authordc.contributor.authorMartinelli, M. 
Authordc.contributor.authorMartins, C. J. A. P. 
Authordc.contributor.authorNesseris, S. 
Authordc.contributor.authorSapone, Domenico 
Authordc.contributor.authorTutusaus, I. 
Authordc.contributor.authorAvgoustidis, A. 
Authordc.contributor.authorCamera, S. 
Authordc.contributor.authorCarbone, C. 
Authordc.contributor.authorCasas, S. 
Authordc.contributor.authorIlic, S. 
Authordc.contributor.authorSakr, Z. 
Authordc.contributor.authorYankelevich, V. 
Authordc.contributor.authorAuricchio, N. 
Authordc.contributor.authorBalestra, A. 
Authordc.contributor.authorBodendorf, C. 
Authordc.contributor.authorBonino, D. 
Authordc.contributor.authorBranchini, E. 
Authordc.contributor.authorBrescia, M. 
Authordc.contributor.authorBrinchmann, J. 
Authordc.contributor.authorCapobianco, V. 
Authordc.contributor.authorCarretero, J. 
Authordc.contributor.authorCastellano, M. 
Authordc.contributor.authorCavuoti, S. 
Authordc.contributor.authorCledassou, R. 
Authordc.contributor.authorCongedo, G. 
Authordc.contributor.authorConversi, L. 
Authordc.contributor.authorCorcione, L. 
Authordc.contributor.authorDubath, F. 
Authordc.contributor.authorEalet, A. 
Authordc.contributor.authorFrailis, M. 
Authordc.contributor.authorFranceschi, E. 
Authordc.contributor.authorFumana, M. 
Authordc.contributor.authorGarilli, B. 
Authordc.contributor.authorGillis, B. 
Authordc.contributor.authorGiocoli, C. 
Authordc.contributor.authorGrupp, F. 
Authordc.contributor.authorHaugan, S. V. H. 
Authordc.contributor.authorHolmes, W. 
Authordc.contributor.authorHormuth, F. 
Authordc.contributor.authorJahnke, K. 
Authordc.contributor.authorKermiche, S. 
Authordc.contributor.authorKilbinger, M. 
Authordc.contributor.authorKitching, T. 
Authordc.contributor.authorKubik, B. 
Authordc.contributor.authorKunz, M. 
Authordc.contributor.authorKurki-Suonio, H. 
Authordc.contributor.authorLigori, S. 
Authordc.contributor.authorLilje, P. B. 
Authordc.contributor.authorLloro, I. 
Authordc.contributor.authorMarggraf, O. 
Authordc.contributor.authorMarkovic, K. 
Authordc.contributor.authorMassey, R. 
Authordc.contributor.authorMei, S. 
Authordc.contributor.authorMeneghetti, M. 
Authordc.contributor.authorMeylan, G. 
Authordc.contributor.authorMoscardini, L. 
Authordc.contributor.authorNiemi, S. 
Authordc.contributor.authorPadilla, C. 
Authordc.contributor.authorPaltani, S. 
Authordc.contributor.authorPasian, F. 
Authordc.contributor.authorPettorino, V. 
Authordc.contributor.authorPires, S. 
Authordc.contributor.authorPolenta, G. 
Authordc.contributor.authorPoncet, M. 
Authordc.contributor.authorPopa, L. 
Authordc.contributor.authorPozzetti, L. 
Authordc.contributor.authorRaison, F. 
Authordc.contributor.authorRhodes, J. 
Authordc.contributor.authorRoncarelli, M. 
Authordc.contributor.authorSaglia, R. 
Authordc.contributor.authorSchneider, P. 
Authordc.contributor.authorSecroun, A. 
Authordc.contributor.authorSerrano, S. 
Authordc.contributor.authorSirignano, C. 
Authordc.contributor.authorSirri, G. 
Authordc.contributor.authorSureau, F. 
Authordc.contributor.authorTaylor, A. 
Authordc.contributor.authorTereno, I. 
Authordc.contributor.authorToledo Moreo, R. 
Authordc.contributor.authorValenziano, L. 
Authordc.contributor.authorVassallo, T. 
Authordc.contributor.authorWang, Y. 
Authordc.contributor.authorWelikala, N. 
Authordc.contributor.authorWeller, J. 
Authordc.contributor.authorZacchei, A. 
Admission datedc.date.accessioned2021-05-31T20:09:52Z
Available datedc.date.available2021-05-31T20:09:52Z
Publication datedc.date.issued2020
Cita de ítemdc.identifier.citationA&A 644, A80 (2020)es_ES
Identifierdc.identifier.other10.1051/0004-6361/202039078
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/179895
Abstractdc.description.abstractContext. In metric theories of gravity with photon number conservation, the luminosity and angular diameter distances are related via the Etherington relation, also known as the distance duality relation (DDR). A violation of this relation would rule out the standard cosmological paradigm and point to the presence of new physics.Aims. We quantify the ability of Euclid, in combination with contemporary surveys, to improve the current constraints on deviations from the DDR in the redshift range 0< z< 1.6.Methods. We start with an analysis of the latest available data, improving previously reported constraints by a factor of 2.5. We then present a detailed analysis of simulated Euclid and external data products, using both standard parametric methods (relying on phenomenological descriptions of possible DDR violations) and a machine learning reconstruction using genetic algorithms.Results. We find that for parametric methods Euclid can (in combination with external probes) improve current constraints by approximately a factor of six, while for non-parametric methods Euclid can improve current constraints by a factor of three.Conclusions. Our results highlight the importance of surveys like Euclid in accurately testing the pillars of the current cosmological paradigm and constraining physics beyond the standard cosmological model.es_ES
Patrocinadordc.description.sponsorshipLa Caixa Foundation 100010434 LCF/BQ/PI19/11690015 Spanish Agencia Estatal de Investigacion through the grant "IFT Centro de Excelencia Severo Ochoa" SEV-2016-0597 FEDER -Fundo Europeu de Desenvolvimento Regional funds through the COMPETE 2020 -Operational Programme for Competitiveness and Internationalisation (POCI) Portuguese funds through FCT -Fundacao para a Ciencia e a Tecnologia POCI-01-0145-FEDER-028987 Centro de Excelencia Severo Ochoa Program SEV-2016-059 Spanish Government RYC-2014-15843 Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT) CONICYT FONDECYT 1200171 Spanish Ministry of Science, Innovation and Universities ESP2017-89838-C3-1-R H2020 programme of the European Commission 776247 UK Research & Innovation (UKRI) Science & Technology Facilities Council (STFC) Science and Technology Development Fund (STDF) ST/P000703/1 European Research Council (ERC) 769130 Academy of Finland European Commission Agenzia Spaziale Italiana (ASI) Belgian Federal Science Policy Office Canadian Euclid Consortium Centre National D'etudes Spatiales Helmholtz Association German Aerospace Centre (DLR) Danish Space Research Institute Portuguese Foundation for Science and Technology European Commission Spanish Government National Aeronautics & Space Administration (NASA) Netherlandse Onderzoekschool Voor Astronomie Norwegian Space Agency Romanian Space Agency State Secretariat for Education, Research and Innovation (SERI) at the Swiss Space O ffice (SSO) United Kingdom Space Agency PGC2018-094773-B-C32es_ES
Lenguagedc.language.isoenes_ES
Publisherdc.publisherEDP Sciences S Aes_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Sourcedc.sourceAstronomy & Astrophysicses_ES
Keywordsdc.subjectCosmology: observationses_ES
Keywordsdc.subjectCosmological parameterses_ES
Keywordsdc.subjectSurveyses_ES
Keywordsdc.subjectMethods: data analysises_ES
Keywordsdc.subjectMethods: statisticales_ES
Keywordsdc.subjectSpace vehicles: instrumentses_ES
Títulodc.titleEuclid: Forecast constraints on the cosmic distance duality relation with complementary external probeses_ES
Document typedc.typeArtículo de revistaes_ES
dcterms.accessRightsdcterms.accessRightsAcceso Abierto
Catalogueruchile.catalogadorcfres_ES
Indexationuchile.indexArtículo de publicación ISI
Indexationuchile.indexArtículo de publicación SCOPUS


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Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile