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Record W4417292294 · doi:10.48550/arxiv.2512.09748

Euclid preparation. Review of forecast constraints on dark energy and modified gravity

2025· preprint· W4417292294 on OpenAlexaff
Euclid Collaboration, N. Frusciante, M. Martinelli, L. Lombriser, Alessandra Silvestri, M. Archidiacono, M. Baldi, N. Bartolo, Emilio Bellini, Giampaolo Benevento, Daniele Bertacca, Camille Bonvin, Benjamin Bose, Philippe Brax, V.F Cardone, Santiago Casas, M.Y Elkhashab, Farbod Hassani, S. Ilić, Katsuhiro Koyama, M Kunz, Fabio Lepori, J. Lesgourgues, C. J. A. P. Martins, David F. Mota, Johannes Noller, F. Pace, D. Paoletti, G. Parimbelli, V. Pettorino, Z. Sakr, Sandhya Srinivasan, Elsa M. Teixeira, I. Tutusaus, Patrick Valageas, H.-A Winther, Julian Adamek, Inês S. Albuquerque, Luís Atayde, Michel-Andrès Breton, S Camera, Chris Carbone, E. Carella, P. Carrilho, F. J. Castander, B. Fiorini, P. Fosalba, Marco Marinucci, Claudio Moretti, Massimo Pietroni, L. Piga, Gabor B. Racz, Francesco Sorrenti, Filippo Vernizzi, C. Viglione, Luca Amendola, S. Andreon, C. Baccigalupi, S Bardelli, R. Bender, A Biviano, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, A. Caillat, J. Carretero, M Castellano, G. Castignani, S. Cavuoti, A. Cimatti, Christopher J. Conselice, L. Conversi, H. M. Courtois, M. Cropper, A. Da Silva, H. Degaudenzi, G. De Lucia, A. M. Di Giorgio, J. Dinis, H. Dole, F Dubath, X. Dupac, S Dusini, A. Ealet, Marcelo Farina, S. Farrens, F Faustini, S. Ferriol, S. Fotopoulou, M. Frailis, E. Franceschi, M. Fumana, B. R. Granett, B Gillis, C. Giocoli, J. Gracia-Carpio, A. Grazian, F. Grupp, S. V. H. Haugan, H. Hoekstra, W. M. Holmes, F. Hormuth, P. Hudelot, K. Jahnke, M Jhabvala, B. Joachimi, S. Kermiche, A. Kiessling, B. Kubik, H Kurki-Suonio, O Lahav, A.M.C Le Brun, S. Ligori, P. B. Lilje, I. Lloro, G Mainetti, D. Maino, E. Maiorano, O Mansutti, O. Marggraf, N. Martinet, F. Marulli, R. Massey, S. Maurogordato, E. Medinaceli, S. Mei, M. Melchior, Y. Mellier, E Merlin, G. Meylan, A Mora, M. Moresco, L Moscardini, C. Neissner, Robert C. Nichol, S. -M. Niemi, J.W Nightingale, C. Padilla, S. Paltani, K. Pedersen, Will J. Percival, S Pires, G. Polenta, Marion Poncet, L. A. Popa, F. Raison, A Renzi, Giovanni Riccio, E. Romelli, R Saglia, Ariel G. Sánchez, D. Sapone, B Sartoris, R. Scaramella, J.A Schewtschenko, M. Schirmer, A Secroun, E. Sefusatti, G. Seidel, M. Seiffert, S Serrano, C Sirignano, G Sirri, A. Spurio Mancini, L. Stanco, J. Steinwagner, P. Tallada-Crespí, D Tavagnacco, A. N. Taylor, N Tessore, F. Torradeflot, L Valenziano, J Valiviita, T. Vassallo, A. Veropalumbo, Yang Wang, J. Weller, A Zacchei, G Zamorani, E. Zucca, E. Bozzo, C. Burigana, M. Calabrese, D. Di Ferdinando, J.A. Escartin Vigo, G. Fabbian, Mohan Harish Maturi, Nuria Mauri, M. Pöntinen, C. Porciani, V. Scottez, M. Tenti, M Viel, M. Wiesmann, Y. Akrami, V. Allevato, S Anselmi, F. Atrio‐Barandela, A. Balaguera-Antolínez, A. Blanchard, Lilian Blot, H. Böhringer, S. Borgani, Michael D. Brown, S Bruton, R. Cabanac, A. Calabro, A Cappi, F Caro, T. Castro, F Cogato, S. Contarini, S. Davini, S. Di Domizio, A.G Ferrari, A. Finoguenov, F. Fornari, L. Gabarra, K. Ganga, J. García-Bellido, V. Gautard, E. Gaztanaga, F. Giacomini, F. Gianotti, G. Gozaliasl, A. Gregorio, María Guidi, C. M. Gutiérrez, A. J. Hall, H. Hildebrandt, J. Hjorth, A. Jiménez Muñoz, Yongtian Kang, Vinay Kansal, C. C. Kirkpatrick, Sergey Kruk, F. Lacasa, M. G. Lattanzi, S. Lee, J Le Graet, L Legrand, Maria Lembo, T.I Liaudat, S. J. Liu, A. Loureiro, J. F. Macías–Pérez, R. Maoli, J. Martín-Fleitas, Louis Maurin, M. Migliaccio, M. Miluzio, P. Monaco, A Montoro, G Morgante, S Nadathur, K. Naidoo, P. Natoli, Luca Pagano, K Paterson, L. Patrizii, Alice Pisani, V. Popa, D. Potter, P. Reimberg, I Risso, P.-F Rocci, M Sahlén, E Sarpa, M. Schultheis, D Sciotti, M. Sereno, Leigh C. Smith, K Tanidis, Chunhui Tao, G. Testera, R Teyssier, A. Troja, M. Tucci, C. Valieri, D. Vergani, G Verza, P Vielzeuf

Bibliographic record

VenueArXiv.org · 2025
Typepreprint
Language
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsSaint Mary's UniversityPerimeter InstituteUniversity of Waterloo
FundersInstitut National de Physique Nucléaire et de Physique des ParticulesScience and Technology Facilities CouncilEuropean Space AgencyAgenzia Spaziale ItalianaFundação para a Ciência e a TecnologiaMagyar Tudományos AkadémiaNational Astronomical Observatory of JapanNorsk RomsenterNorges ForskningsrådAgenția Spațială RomânăSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungEuropean CommissionNational Aeronautics and Space AdministrationDeutsche Forschungsgemeinschaft
KeywordsDark energyDark matterGeneral relativityWeak gravitational lensingLambda-CDM modelGravitationCosmologyCosmological perturbation theoryObservable

Abstract

fetched live from OpenAlex

The Euclid mission has been designed to provide, as one of its main deliverables, information on the nature of the gravitational interaction, which determines the expansion of the Universe and the formation of structures. Thus, Euclid has the potential to test deviations from general relativity that will allow us to shed light on long-lasting problems in the standard cosmological model, $Λ$CDM. Euclid will mainly do this by using two complementary probes: weak gravitational lensing and galaxy clustering. In this paper we review pre-launch Euclid analyses for dark energy and modified gravity. These include forecast constraints with future Euclid data on cosmological parameters for different cosmological models, such as a time-varying dark energy component, phenomenological modifications of the perturbation sector and specific modified gravity models, with further extensions that include neutrino physics and the coupling to the electromagnetic sector through the fine-structure constant. We review the study of the impact of nonlinear clustering methods on beyond-$Λ$CDM constraints with Euclid. This is of fundamental importance to efficiently predict the large-scale clustering of matter and dark matter halos, given that we will have access to a wealth of information on scales beyond the linear regime. We inspect the extension of theoretical predictions for observable quantities in alternative cosmologies to $Λ$CDM at fully nonlinear scales by means of $N$-body simulations. We discuss the impact of relativistic corrections in extended cosmological models. Overall, this review highlights the significant potential of the Euclid mission to tightly constrain parameters of dark energy and modified gravity models, or perhaps to detect possible signatures of a $Λ$CDM failure.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: Theoretical or conceptual
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.114
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.000
Science and technology studies0.0000.001
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.029
GPT teacher head0.301
Teacher spread0.272 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

Study designTheoretical or conceptual
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations0
Published2025
Admission routes1
Has abstractyes

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