Observational challenges for the standard FLRW model

Author:

Buchert Thomas1,Coley Alan A.2,Kleinert Hagen3,Roukema Boudewijn F.14,Wiltshire David L.5

Affiliation:

1. Université de Lyon, Observatoire de Lyon, Centre de Recherche Astrophysique de Lyon, CNRS UMR 5574: Université Lyon 1 and, École Normale Supérieure de Lyon, 9 Avenue Charles André, F-69230 Saint-Genis-Laval, France

2. Department of Mathematics and Statistics, Dalhousie University, Halifax, Canada, NS B3H 3J5, Canada

3. Institute for Theoretical Physics, Freie Universität Berlin, Arnimallee 14, 14195 Berlin, Germany

4. Toruń Centre for Astronomy, Faculty of Physics, Astronomy and Informatics, Grudziadzka 5, Nicolaus Copernicus University, ul. Gagarina 11, 87-100 Toruń, Poland

5. Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch 8140, New Zealand

Abstract

In this paper, we summarize some of the main observational challenges for the standard Friedmann–Lemaître–Robertson–Walker (FLRW) cosmological model and describe how results recently presented in the parallel session “Large-scale Structure and Statistics” (DE3) at the “Fourteenth Marcel Grossman Meeting on General Relativity” are related to these challenges.

Publisher

World Scientific Pub Co Pte Lt

Subject

Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics

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