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Black hole scalarisation from the breakdown of scale-invariance

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Academic year: 2021

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FIG. 3. The profile functions (left panel) of a typical GMGHS solution and (right panel) its scalarized version for the same global charges.
FIG. 4. Variation of the reduced scalar charge with (main panel) the ratio of the ADM mass to the mass of the scalarized solution at the bifurcation point, and (inset) the electric charge to mass ratio, q.
FIG. 5. The domain of existence of RN-F 4 BHs with Q ¼ Q m in a (main panel) reduced temperature or (inset) reduced area vs charge to mass ratio, q, plot.
FIG. 6. l ¼ 0 , 1, 2 existence lines for the RN-F 4 solution with Q ¼ Q m ¼ 1 . The inset enlarges the region of small j ξ j.
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