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Record W4381832831 · doi:10.48550/arxiv.2306.12368

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

2023· preprint· en· W4381832831 on OpenAlexaff
Noemi Frusciante, F. Pace, V. F. Cardone, S. 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, L. Lombriser, D. Paoletti, Massimo Pietroni, Alberto Rozas-Fernández, Z. Sakr, A. Silvestri, Filippo Vernizzi, Hans A. Winther, N. Aghanim, L. Amendola, N. Auricchio, R. Azzollini, M Baldi, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, V. Capobianco, C. Carbone, J. Carretero, M Castellano, S. Cavuoti, A. Cimatti, R. Clédassou, G. Congedo, L Conversi, Y. Copin, L. Corcione, F. Courbin, 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, Frank Grupp, L. Guzzo, S. V. H. Haugan, W. Holmes, F. Hormuth, A. Hornstrup, K. Jahnkę, 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. Popa, F. Raison, R. Rébolo, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, R. Saglia, D. Sapone, B Sartoris, A. Secroun, G. Seidel, C. Sirignano, G Sirri, L. Stanco, C. Surace, 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

VenuearXiv (Cornell University) · 2023
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicSolar and Space Plasma Dynamics
Canadian institutionsUniversity of Waterloo
FundersHorizon 2020 Framework ProgrammeAgenția Spațială RomânăNorsk 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 RicercaSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungStaatssekretariat für Bildung, Forschung und InnovationDeutsche ForschungsgemeinschaftEuropean CommissionNational Aeronautics and Space AdministrationMinisterio de Ciencia, Innovación y UniversidadesFundação para a Ciência e a TecnologiaDipartimenti di Eccellenza
KeywordsPhysicsOmegaGeneral relativityGalaxyAstrophysicsWeak gravitational lensingCosmologyDark energyGravitationMathematical physicsRedshiftClassical mechanicsQuantum mechanics

Abstract

fetched live from OpenAlex

The future Euclid space satellite mission will offer an invaluable opportunity to constrain modifications to Einstein's general relativity at cosmic scales. 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. We considered three specific models, namely JBD, a scalar-tensor theory with a flat potential, the 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 (KM) 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, $ω_{\rm BD}$, $Ω_{\rm rc}$ and $ε_{2,0}$. 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. In an optimistic setting at 68.3\% confidence interval, we find the following percentage relative errors with Euclid alone: for $\log_{10}{ω_{\rm BD}}$, with a fiducial value of $ω_{\rm BD}=800$, 27.1\% using GCsp alone, 3.6\% using GCph+WL+XC and 3.2\% using GCph+WL+XC+GCsp; for $\log_{10}{Ω_{\rm rc}}$, with a fiducial value of $Ω_{\rm rc}=0.25$, we find 93.4\%, 20\% and 15\% respectively; and finally, for $ε_{2,0}=-0.04$, we find 3.4\%, 0.15\%, and 0.14\%. (abridged)

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)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation 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 score0.217
Threshold uncertainty score0.753

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.001
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 head0.045
GPT teacher head0.192
Teacher spread0.148 · 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.

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

Citations1
Published2023
Admission routes1
Has abstractyes

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