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Statut |
Confirmé |
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Série |
SEM-GRECO |
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Domaines |
astro-ph |
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Date |
Lundi 2 Mars 2015 |
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Heure |
11:00 |
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Institut |
IAP |
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Salle |
Salle des séminaires Évry Schatzman |
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Nom de l'orateur |
Florent |
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Prenom de l'orateur |
Leclercq |
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Addresse email de l'orateur |
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Institution de l'orateur |
Institut d'Astrophysique de Paris |
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Titre |
Bayesian large-scale structure inference and cosmic web analysis |
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Résumé |
Ideally, cosmological surveys should be analyzed in terms of the joint constraints they place on the initial conditions from which structure originates and on their subsequent gravitational evolution. In this talk, I will describe an innovative statistical data analysis approach designed for the ab initio simultaneous analysis of the formation history and morphology of the large-scale structure of the inhomogeneous Universe.
As three-dimensional large-scale structure surveys contain a wealth of information that cannot be trivially extracted due to the non-linear dynamical evolution of the density field, I will discuss methods designed to improve upon previous techniques by including non-Gaussian and non-linear data models for the description of late-time structure formation.
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Numéro de preprint arXiv |
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Commentaires |
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Fichiers attachés |
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