Instability of the massive Klein-Gordon field on the Kerr spacetime
May, 2007Citations per year
Abstract: (arXiv)
We investigate the instability of the massive scalar field in the vicinity of a rotating black hole. The instability arises from amplification caused by the classical superradiance effect. The instability affects bound states: solutions to the massive Klein-Gordon equation which tend to zero at infinity. We calculate the spectrum of bound state frequencies on the Kerr background using a continued fraction method, adapted from studies of quasinormal modes. We demonstrate that the instability is most significant for the , state, for . For a fast rotating hole () we find a maximum growth rate of , at . The physical implications are discussed.- 04.70.-s
- field theory: scalar
- black hole: rotation
- space-time: Kerr
- bound state: spectrum
- tensor: energy-momentum
- Klein-Gordon equation: massive
- bound state: decay
- stability
- superradiance
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