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Fig. 7.

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Entropy evolution of a 1.3 × 1015M mass non-cool-core cluster, a 1.6 × 1015M cool-core cluster, a 1.6 × 1013M size group, and a 0.91 × 1012M halo, from left to right. The black circle indicates the virial radius of each object. The box lengths are scaled to ten times the virial radius for the clusters and 40 times the virial radius for the groups or galaxies with a slice thickness of 1 Mpc/h for all images.

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