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Record W4403138712 · doi:10.1051/0004-6361/202347526

<i>Euclid</i>: Constraining linearly scale-independent modifications of gravity with the spectroscopic and photometric primary probes

2024· article· en· W4403138712 on OpenAlexaff
Noemi Frusciante, Francesco Pace, V. F. Cardone, Santiago Casas, I. Tutusaus, M. Ballardini, Emilio Bellini, Giampaolo Benevento, Benjamin Bose, Patrick Valageas, N. Bartolo, Philippe Brax, A. Finoguenov, F. Finelli⋆, K. Koyama, L. Legrand, Lucas Lombriser, D. Paoletti, Massimo Pietroni, Alberto Rozas-Fernández, Z. Sakr, Alessandra Silvestri, Filippo Vernizzi, Hans A. Winther, N. Aghanim, L. Amendola, N. Auricchio, R. Azzollini, Marco Baldi, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, V. Capobianco, C. Carbone, J. Carretero, M. Castellano, S. Cavuoti, A. Cimatti, R. Cledassou, G. Congedo, L. Conversi, Y. Copin, L. Corcione, F. Courbin, M. Cropper, A. Da Silva, H. Degaudenzi, J. Dinis, F. Dubath, X Dupac, S. Dusini, S. Farrens, S. Ferriol, P. Fosalba, M. Frailis, E. Franceschi, S. Galeotta, B. Gillis, C. Giocoli, A. Grazian, F. Grupp, L. Guzzo, S. V. H. Haugan, W. A. Holmes, F. Hormuth, A. Hornstrup, A. Bongiorno, S. Kermiche, A. Kiessling, M. Kilbinger, T. Kitching, M. Kunz, H. Kurki‐Suonio, S. Ligori, P. B. Lilje, I. Lloro, E Maiorano, O. Mansutti, O. Marggraf, K. Markovič, F. Marulli, R. Massey, E. Medinaceli, M. Meneghetti, G. Meylan, M. Moresco, L. Moscardini, E. Munari, S. M. Niemi, J.W Nightingale, S. Paltani, F. Pasian, K. Pedersen, W.J Percival, V. Pettorino, G. Polenta, M. Poncet, L. A. Popa, F. Raison, R. Rébolo, A. Renzi, Jason Rhodes, G. Riccio, E. Romelli, R. P. Saglia, D. Sapone, B. Sartoris, A. Secroun, G. Seidel, C. Sirignano, G. Sirri, L. Stančo, P. Tallada-Crespí, A. N. Taylor, I. Tereno, R. Toledo-Moreo, F. Torradeflot, E. A. Valentijn, L. Valenziano, T. Vassallo, G. A. Verdoes Kleijn, Yun Wang, A. Zacchei, G. Zamorani, J. Zoubian, V. Scottez

Bibliographic record

VenueAstronomy and Astrophysics · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsPerimeter InstituteUniversity of Waterloo
FundersNorsk RomsenterNational Astronomical Observatory of JapanUniversidade de LisboaMinisterio de Ciencia e InnovaciónNational Science FoundationEuropean Space AgencyAgenzia Spaziale ItalianaScience and Technology Facilities CouncilMinistero dell’Istruzione, dell’Università e della RicercaHorizon 2020 Framework ProgrammeAgenția Spațială RomânăAcademy of FinlandSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungStaatssekretariat für Bildung, Forschung und InnovationIstituto Nazionale di Fisica NucleareDeutsche ForschungsgemeinschaftEuropean CommissionNational Aeronautics and Space AdministrationMinisterio de Ciencia, Innovación y UniversidadesFundação para a Ciência e a TecnologiaDipartimenti di Eccellenza
KeywordsPhysicsGeneral relativityCosmologyTheoretical physicsPlanckMinkowski spaceMatter power spectrumGalaxyAstrophysicsDark energyMathematical physics

Abstract

fetched live from OpenAlex

Context. The future Euclid space satellite mission will offer an invaluable opportunity to constrain modifications to Einstein’s general relativity at cosmic scales. In this paper, we focus on modified gravity models characterised, at linear scales, by a scale-independent growth of perturbations while featuring different testable types of derivative screening mechanisms at smaller non-linear scales. Aims. We considered three specific models, namely Jordan-Brans-Dicke, a scalar-tensor theory with a flat potential, the normal branch of Dvali-Gabadadze-Porrati (nDGP) gravity, a braneworld model in which our Universe is a four-dimensional brane embedded in a five-dimensional Minkowski space-time, and k-mouflage gravity, an extension of k-essence scenarios with a universal coupling of the scalar field to matter. In preparation for real data, we provide forecasts from spectroscopic and photometric primary probes by Euclid on the cosmological parameters and the additional parameters of the models, respectively, ωBD, Ωгc and ϵ2,0, which quantify the deviations from general relativity. This analysis will improve our knowledge of the cosmology of these modified gravity models. Methods. The forecast analysis employs the Fisher matrix method applied to weak lensing (WL); photometric galaxy clustering (GCph), spectroscopic galaxy clustering (GCsp) and the cross-correlation (XC) between GCph and WL. For the Euclid survey specifications, we define three scenarios that are characterised by different cuts in the maximum multipole and wave number, to assess the constraining power of non-linear scales. For each model we considered two fiducial values for the corresponding model parameter. Results. In an optimistic setting at 68.3% confidence interval, we find the following percentage relative errors with Euclid alone: for log10 ωBD, with a fiducial value of ωBD = 800, 27.1% using GCsp alone, 3.6% using GCph+WL+XC and 3.2% using GCph+WL+XC+GCsp; for log10 Ωгc, with a fiducial value of Ωгc = 0.25, we find 93.4, 20 and 15% respectively; and finally, for ϵ2,0 = −0.04, we find 3.4%, 0.15%, and 0.14%. From the relative errors for fiducial values closer to their ΛCDM limits, we find that most of the constraining power is lost. Our results highlight the importance of the constraining power from non-linear scales.

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 machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.002
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.011
Threshold uncertainty score0.022

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.001
Scholarly communication0.0010.001
Open science0.0000.001
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0010.000

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 head0.006
GPT teacher head0.225
Teacher spread0.219 · 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 source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
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

Citations14
Published2024
Admission routes1
Has abstractyes

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