Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes
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2020Metadata
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Martinelli, M.
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Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes
Author
- Martinelli, M.;
- Martins, C. J. A. P.;
- Nesseris, S.;
- Sapone, Domenico;
- Tutusaus, I.;
- Avgoustidis, A.;
- Camera, S.;
- Carbone, C.;
- Casas, S.;
- Ilic, S.;
- Sakr, Z.;
- Yankelevich, V.;
- Auricchio, N.;
- Balestra, A.;
- Bodendorf, C.;
- Bonino, D.;
- Branchini, E.;
- Brescia, M.;
- Brinchmann, J.;
- Capobianco, V.;
- Carretero, J.;
- Castellano, M.;
- Cavuoti, S.;
- Cledassou, R.;
- Congedo, G.;
- Conversi, L.;
- Corcione, L.;
- Dubath, F.;
- Ealet, A.;
- Frailis, M.;
- Franceschi, E.;
- Fumana, M.;
- Garilli, B.;
- Gillis, B.;
- Giocoli, C.;
- Grupp, F.;
- Haugan, S. V. H.;
- Holmes, W.;
- Hormuth, F.;
- Jahnke, K.;
- Kermiche, S.;
- Kilbinger, M.;
- Kitching, T.;
- Kubik, B.;
- Kunz, M.;
- Kurki-Suonio, H.;
- Ligori, S.;
- Lilje, P. B.;
- Lloro, I.;
- Marggraf, O.;
- Markovic, K.;
- Massey, R.;
- Mei, S.;
- Meneghetti, M.;
- Meylan, G.;
- Moscardini, L.;
- Niemi, S.;
- Padilla, C.;
- Paltani, S.;
- Pasian, F.;
- Pettorino, V.;
- Pires, S.;
- Polenta, G.;
- Poncet, M.;
- Popa, L.;
- Pozzetti, L.;
- Raison, F.;
- Rhodes, J.;
- Roncarelli, M.;
- Saglia, R.;
- Schneider, P.;
- Secroun, A.;
- Serrano, S.;
- Sirignano, C.;
- Sirri, G.;
- Sureau, F.;
- Taylor, A.;
- Tereno, I.;
- Toledo Moreo, R.;
- Valenziano, L.;
- Vassallo, T.;
- Wang, Y.;
- Welikala, N.;
- Weller, J.;
- Zacchei, A.;
Abstract
Context. 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.
Patrocinador
La 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-C32
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Artículo de publicación ISI Artículo de publicación SCOPUS
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A&A 644, A80 (2020)
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