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Massive complex scalar field in the Kerr-Sen geometry: Exact solution of wave equation and Hawking radiation

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arxiv gr-qc/0303075 v1 pith:ERWPJZJ3 submitted 2003-03-20 gr-qc

S. Q. Wu , X. Cai This is my paper · ORCID
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keywords equationblackholekerr-senscalarwavecomplexgeometry
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The separated radial part of a massive complex scalar wave equation in the Kerr- Sen geometry is shown to satisfy the generalized spheroidal wave equation which is, in fact, a confluent Heun equation up to a multiplier. The Hawking evaporation of scalar particles in the Kerr-Sen black hole background is investigated by the Damour-Ruffini-Sannan method. It is shown that quantum thermal effect of the Kerr-Sen black hole has the same character as that of the Kerr-Newman black hole.

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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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