Scalar clouds around Kerr–Sen black holes

DOI10.1088/1361-6382/aa7964zbMath1373.83059arXiv1706.04441OpenAlexW3098441493MaRDI QIDQ4592661

Dao-Jun Liu, Xiang-Hua Zhai, Yang Huang, Xin-Zhou Li

Publication date: 7 November 2017

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1706.04441

zbMATH Keywords

scalar fieldKerr-Sen black holeextremal Kerr-Newman backgroundstationary resonances

Mathematics Subject Classification ID

Black holes (83C57) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (7)

Accelerating black holes in the low energy heterotic string theory ⋮ Relaxation rate of RNdS black hole ⋮ The fastest relaxation rate of higher-dimensional Reissner-Nordström black hole ⋮ Charged black holes in non-linear Q-clouds with O(3) symmetry ⋮ Black holes with synchronised Proca hair: linear clouds and fundamental non-linear solutions ⋮ Black holes, stationary clouds and magnetic fields ⋮ Massive vector fields in Kerr-Newman and Kerr-Sen black hole spacetimes

Uses Software

• DLMF

Cites Work

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• Rotating charged black hole solution in heterotic string theory
• Instability of Massive Scalar Fields in Kerr-Newman Spacetime
• Massive complex scalar field in the Kerr–Sen geometry: Exact solution of wave equation and Hawking radiation
• A new spin on black hole hair

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