Fig. 5.

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Predicted entropy profile for a halo mass of 1013 M⊙ (left panel), 1014 M⊙ (central panel), and 1015 M⊙ (right panel). The radius has been normalized to the shock (virial) radius. All profiles are normalized at the shock radius. In red we plot a reference powerlaw with slope 1.2, in blue the profile derived from a combination of the functional forms: K(R) = Kv(Mh(R)) and in black the one derived by solving the hydrostatic equilibrium equation.
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