A proof that dyonic-like dilatonic black holes have a unique innermost stable circular orbit, plus explicit ISCO formulas for selected values of the dilaton coupling parameter.
Such analysis offers valuable in- sight into the nature of these objects and their influence on the surrounding spacetime
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Stability Analysis of Circular Geodesics in Dyonic Dilatonic Black Hole Spacetimes
A proof that dyonic-like dilatonic black holes have a unique innermost stable circular orbit, plus explicit ISCO formulas for selected values of the dilaton coupling parameter.