2018/09/11 by Matteo Cataneo, David Rapetti · 1 citation
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Galaxy formation and evolution #General relativity #Gravitation #Observable #Physics #Theoretical physics #astro-ph.CO
paper · pdf · doi:10.1142/s0218271818480061
published as International Journal of Modern Physics D, Vol. 27, No. 15, 1848006 (2018) · 45 pages, 11 figures. This is a pre-referee version of the article published as part of the special issue "Modified Gravity: Progresses and Outlook of Theories, Numerical Techniques and Observational Tests". To read its accepted version and to access the other review articles of the special issue visit https://www.worldscientific.com/toc/ijmpd/27/15
openalex publication_date 2018/09/11 · arxiv created 2019/02/26 · arxiv updated 2019/02/27 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Changes in the law of gravity have far-reaching implications for the formation and evolution of galaxy clusters, and appear as peculiar signatures in their mass-observable relations, structural properties, internal dynamics, and abundance. We review the outstanding progress made in recent years towards constraining deviations from General Relativity with galaxy clusters, and give an overview of the yet untapped information becoming accessible with forthcoming surveys that will map large portions of the sky in great detail and unprecedented depth.