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Fig. 8.

Fig. 8. Refer to the following caption and surrounding text.

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Ratio of surviving to initial GCs within the central region of galaxies delimited by the scale radius rs of halos as a function of the mass ratio Mhalo/MGC and for different FDM particle masses m22. The survival criterion corresponds to a final apocentre larger than 0.1 rs. The left panel shows an in situ population ( r apo init < r s Mathematical equation: $ r_{\mathrm{apo}}^{\mathrm{init}} < r_s $) initially composed of about N0 = 300 GCs, while the right panel corresponds to an ex situ population ( 3 r s < r apo init < 10 r s Mathematical equation: $ 3r_s < r_{\mathrm{apo}}^{\mathrm{init}} < 10r_s $) initially composed of about N0 = 2100 GCs.

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