Quasi-bound states of massive scalar fields in the Kerr black-hole spacetime: beyond the hydrogenic approximation

DOI10.1016/j.physletb.2015.07.071zbMath1364.83021arXiv1510.05649OpenAlexW1867686091MaRDI QIDQ2396536

Shahar Hod

Publication date: 8 June 2017

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1510.05649

Mathematics Subject Classification ID

Black holes (83C57)

Related Items (8)

Kerr-Newman black holes with scalar hair ⋮ Spinning Kerr black holes with stationary massive scalar clouds: the large-coupling regime ⋮ Black holes with synchronised Proca hair: linear clouds and fundamental non-linear solutions ⋮ Generalized Schrödinger equations with quadratical energy-dependence in the potential: Darboux transformations and application to the Heun class ⋮ Black holes, stationary clouds and magnetic fields ⋮ Stationary scalar clouds around a BTZ black hole ⋮ Quasibound states of the Dirac field in Schwarzschild and Reissner–Nordström black hole backgrounds ⋮ Inside black holes with synchronized hair

Cites Work

• Unnamed Item
• Stationary scalar configurations around extremal charged black holes
• Black holes as particle detectors: evolution of superradiant instabilities
• Classes of exact solutions to the Teukolsky master equation
• Maximal Analytic Extension of the Kerr Metric

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