The Shape of the Chameleon Fifth-Force on the Mass Components of Galaxy Clusters

The Shape of the Chameleon Fifth-Force on the Mass Components of Galaxy Clusters

In the context of chameleon gravity, we present a semi-analytical solution of the chameleon field profile in an accurately modelled galaxy cluster’s mass components, namely the stellar mass of the Brightest Cluster Galaxy (BCG), the baryonic mass in galaxies other than the BCG, the mass of the Intra...

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Bibliographic Details
Main Authors: Lorenzo Pizzuti, Valentina Amatori, Alexandre M. Pombo, Sandeep Haridasu
Format: Article
Language:English
Published: MDPI AG 2024-11-01
Series:Universe
Subjects:
modified gravity
galaxy clusters
cosmology
Online Access:https://www.mdpi.com/2218-1997/10/12/443
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https://www.mdpi.com/2218-1997/10/12/443

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