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Large scale structures and the cubic galileon model
Published 30 Dec 2015 in gr-qc and astro-ph.CO | (1512.08856v2)
Abstract: The maximum size of a bound cosmic structure is computed perturbatively as a function of its mass in the framework of the cubic galileon, proposed recently to model the dark energy of our Universe. Comparison of our results with observations constrains the matter-galileon coupling of the model to , thus improving previous bounds based solely on solar system physics.
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