Aller au contenu principal
Accès ouvert déclaré 2025 article

Euclid : An emulator for baryonic effects on the matter bispectrum

3Citations signalées, ce qui n’est pas une note de qualité
119Institutions déclarées
20Pays d’affiliation déclarés

Rattachement africain : ca, ch, it, at, es, nl, gb, de, ru, rs, us, fr, pt, no, dk, fi, lb, ro, cl, sk. Niveau de preuve : code pays fourni par la source.

Le résumé fourni par la source

The Euclid mission and other next-generation large-scale structure surveys will enable high-precision measurements of the cosmic matter distribution. Understanding the impact of baryonic processes such as star formation and active galactic nuclei (AGN) feedback on matter clustering is crucial to ensure precise and unbiased cosmological inference. Most theoretical models of baryonic effects to date focus on two-point statistics, neglecting higher-order contributions. This work develops a fast and accurate emulator for baryonic effects on the matter bispectrum, a key non-Gaussian statistic in the nonlinear regime. We employ high-resolution N -body simulations from the BACCO suite and apply a combination of cutting-edge techniques such as cosmology scaling and baryonification to efficiently span a large cosmological and astrophysical parameter space. A deep neural network is trained to emulate baryonic effects on the matter bispectrum measured in simulations, capturing modifications across various scales and redshifts relevant to Euclid . We validate the emulator accuracy and robustness using an analysis of Euclid mock data, employing predictions from the state-of-the-art FLAMINGO hydrodynamical simulations. The emulator reproduces baryonic suppression in the bispectrum to better than 2% for the 68% percentile across most triangle configurations for k ∈ [0.01, 20] h Mpc −1 and ensures consistency between cosmological posteriors inferred from second- and third-order weak lensing statistics. These results demonstrate that our emulator meets the high-precision requirements of the Euclid mission for at least the first data release and provides reliable forecasts of the cosmological information contained in the small-scale matter bispectrum. This underscores the potential of emulation techniques to bridge the gap between complex baryonic physics and observational data, maximising the scientific output of Euclid .

Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.

Le contrôle bibliographique ouvert

DOI retrouvé dans Crossref DOI retrouvé, mais le titre doit être comparé manuellement.

Titre Crossref
<i>Euclid</i> : An emulator for baryonic effects on the matter bispectrum
Date Crossref
01/01/2026
Éditeur
EDP Sciences
Type
journal-article

Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.

Les institutions déclarées

University of WaterlooUniversity of ZurichIstituto Nazionale di Fisica Nucleare, Sezione di BolognaUniversität InnsbruckIkerbasqueDonostia International Physics CenterLeiden UniversityUniversity of OxfordUniversity of CambridgeMax Planck Institute for Extraterrestrial PhysicsInstitute of AstronomyAstronomical ObservatoryUniversity of BonnPerimeter InstituteUniversity of SurreyBrera Astronomical ObservatoryScuola Internazionale Superiore di Studi AvanzatiTrieste Astronomical ObservatoryIstituto Nazionale di Fisica Nucleare, Sezione di TriesteInstitute for Fundamental Physics of the UniverseOsservatorio astronomico di BolognaOsservatorio di Astrofisica e Scienza dello SpazioUniversity of BolognaOsservatorio Astronomico di PadovaIstituto Nazionale di Fisica Nucleare, Sezione di GenovaUniversity of GenoaAstronomical Observatory of CapodimonteFederico II University HospitalIstituto Nazionale di Fisica Nucleare, Sezione di TorinoOsservatorio Astrofisico di TorinoUniversity of TurinNational Institute for AstrophysicsAstronomical Observatory of RomeIstituto Nazionale di Fisica Nucleare, Sezione di Roma IPort d'Informació CientíficaCentro de Investigaciones Energéticas, Medioambientales y TecnológicasRWTH Aachen UniversityIstituto Nazionale di Fisica Nucleare, Sezione di NapoliNaples Anesthesia & Physician AssociatesUniversity of Hawaii SystemInstituto de Astrofísica de CanariasRoyal ObservatoryUniversity of EdinburghEuropean Space AgencyEuropean Space Astronomy CentreEuropean Space Research InstituteLyon 1 UniversitéCentre National de la Recherche ScientifiqueInstitute of Nuclear Physics of LyonInstitut de Physique des 2 Infinis de LyonInstitució Catalana de Recerca i Estudis AvançatsInstitut Català de Ciències del ClimaLyon CollegeUniversity of LisbonInstitute of Astrophysics and Space SciencesUniversity of GenevaAix-Marseille UniversitéLaboratoire d’Astrophysique de MarseilleChâteau GombertSKA ObservatoryIstituto Nazionale di Fisica Nucleare, Sezione di PadovaCentre de physique des particules de MarseilleInstitute for Space Astrophysics and PlanetologyInstitute of Space SciencesInstitut d'Estudis Espacials de CatalunyaLudwig-Maximilians-Universität MünchenUniversity of OsloJet Propulsion LaboratoryLancaster UniversityFelix ScholarshipDAWN Center for Independent LivingTechnical University of DenmarkMax Planck Institute for AstronomyGoddard Space Flight CenterUniversity College LondonUniversité Paris CitéCommissariat à l'Énergie Atomique et aux Énergies AlternativesUniversité Paris-SaclayAstrophysique, Instrumentation et ModélisationCEA Paris-SaclayLaboratoire de Physique ThéoriqueUniversity of HelsinkiHelsinki Institute of PhysicsUniversité Paris Sciences et LettresObservatoire de ParisSorbonne UniversitéLaboratoire Univers et ThéoriesCentre de Calcul de l’Institut National de Physique Nucléaire et de Physique des ParticulesUniversity of MilanIstituto Nazionale di Fisica Nucleare, Sezione di MilanoInternational University of BeirutFHNW University of Applied Sciences and Arts Northwestern SwitzerlandÉcole Polytechnique Fédérale de LausanneInstitute for High Energy PhysicsEuropean Space Research and Technology CentreUniversity of CopenhagenUnited Kingdom Space AgencyCentre National d'Études SpatialesInstitute of Space Science - INFLPR SubsidiaryUniversity of PaduaUniversité Toulouse III - Paul SabatierUniversity of Saint JosephHeidelberg UniversitySt. Joseph Medical CenterInstitut de Recherche en Astrophysique et PlanétologieHeidelberg Institute for Theoretical StudiesUniversity of ChilePark UniversityRoyal Holloway University of LondonUniversidad Politécnica de CartagenaUniversity of GroningenAstronomical Institute of the Slovak Academy of SciencesCalifornia Institute of TechnologyInfrared Processing and Analysis CenterIstituto di Radioastronomia di BolognaUniversité Catholique de LilleUniversité de LilleInstitut d'Astrophysique de ParisComputing Center

Une affiliation ne permet pas de déduire la nationalité d’un auteur.

Les sujets associés

Cosmology and Gravitation TheoriesComputational Physics and Python ApplicationsAstronomy and Astrophysical Research

BNTIC News n’est pas le producteur de ces données. Les publications sont interrogées à la demande dans Crossref, OpenAIRE, DOAJ, Europe PMC, HAL, DataCite, AfricArXiv, ROR et la Banque mondiale, sans clé d’accès. OpenAlex reste optionnel. Aucun service payant n’est nécessaire et aucune donnée externe n’est enregistrée en base. Consulter les sources et leurs limites.