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

DOI10.1063/1.1539899zbMath1061.83032arXivgr-qc/0303075OpenAlexW2952312434MaRDI QIDQ4832931

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Publication date: 14 December 2004

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0303075

Mathematics Subject Classification ID

Black holes (83C57) Methods of quantum field theory in general relativity and gravitational theory (83C47)

Related Items (13)

Heun equation, Teukolsky equation, and type-D metrics ⋮ Observing the contour profile of a Kerr–Sen black hole ⋮ Scalar clouds around Kerr–Sen black holes ⋮ Radiation fluxes of gravitational, electromagnetic, and scalar perturbations in type-D black holes: an exact approach ⋮ Динамика волнового пакета в окрестностях горизонта событий черной дыры ⋮ A matrix method for quasinormal modes: Kerr and Kerr–Sen black holes ⋮ Hawking radiation of the Kerr-Sen black hole via tunneling ⋮ Generalized hidden symmetries and the Kerr-Sen black hole ⋮ Four five-parametric and five four-parametric independent confluent Heun potentials for the stationary Klein-Gordon equation ⋮ HAWKING RADIATION OF FERMIONS FOR THE KERR–SEN DILATON–AXION BLACK HOLE ⋮ CHARACTERISTICS OF QUANTUM RADIATION OF SLOWLY VARYING NONSTATIONARY KERR–NEWMAN BLACK HOLES ⋮ Solution of the Dirac equation in the rotating Bertotti–Robinson spacetime ⋮ Quantum radiation properties of Dirac particles in general nonstationary black holes

Cites Work

• Solutions to a spheroidal wave equation
• Exact solutions to sourceless charged massive scalar field equation on Kerr–Newman background
• Rotating charged black hole solution in heterotic string theory
• Black hole explosions?

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