Charged particle orbits around GMGHS dilaton black holes transition from ordered to chaotic as the black hole charge or magnetic charge parameter increases.
Connections between the shadow radius and the quasinormal modes of Kerr-Sen black hole
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The correspondence between the shadow radius and the quasi-normal modes of the Kerr-Sen black hole is studied. By using the equation of the shadow radius of the Kerr-Sen black hole and the angular separation constant of the quasi-normal modes, the expression of the real part of quasi-normal modes related to the shadow radius is obtained. We found that in the eikonal limit, our formula coincides with the previous result. Moreover, we also calculate the energy emission rate of the Kerr-Sen black hole, it turns out that the peak energy emissivity is inversely correlated with the charge parameter.
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Chaos dynamics of charged particles near Gibbons-Maeda-Garfinkle-Horowitz-Strominger black holes
Charged particle orbits around GMGHS dilaton black holes transition from ordered to chaotic as the black hole charge or magnetic charge parameter increases.