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Charged scalar fields in a Kerr-Sen black hole: exact solutions, Hawking radiation, and resonant frequencies

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arxiv 1811.06129 v2 pith:W5E6MNTB submitted 2018-11-15 gr-qc

classification gr-qc
keywords frequenciesresonantchargedexactfieldshawkingkerr-senradial
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In this study, we consider charged massive scalar fields around a Kerr-Sen spacetime. The radial and angular parts of the covariant Klein-Gordon equation are solved in terms of the confluent Heun function. From the exact radial solution, we obtain the Hawking radiation spectrum and discuss its resonant frequencies. The massless case of the resonant frequencies is also examined.

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  1. Chaos dynamics of charged particles near Gibbons-Maeda-Garfinkle-Horowitz-Strominger black holes

    hep-th 2025-07 reject novelty 4.0 of 10

    Charged particle orbits around GMGHS dilaton black holes transition from ordered to chaotic as the black hole charge or magnetic charge parameter increases.

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