Median temperature ratios and gas temperature as a function of distance from the halo center. From top to bottom, each row shows the median ratio of the final (i.e., after implementing our model) and the halo virial temperature, the median ratio of the final gas temperature and the gas temperature when only our cooling model is applied, and the median gas temperature. All as a function of distance from the halo center, expressed as a fraction of the virial radius. Each column from left to right corresponds to considering PBHs with masses of 1, 33, and 100 M_⊙, with different fractions of DM composed of these PBHs, as indicated in each panel. For reference, we include the case of f_PBH = 0, where we applied our cooling model alone. The error bars represent the standard deviation in each distance bin. Individual profiles were first calculated around each halo separately, and then the median values of the temperature ratios were derived from these individual profiles of the six halos. The virial temperatures range from 3800 to 8800 K.