Instability of the massive Klein-Gordon field on the Kerr spacetime

May, 2007
27 pages
Published in:
  • Phys.Rev.D 76 (2007) 084001
e-Print:

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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 l=1l = 1, m=1m = 1 state, for Mμ0.5M \mu \lesssim 0.5. For a fast rotating hole (a=0.99a = 0.99) we find a maximum growth rate of τ11.5×107(GM/c3)1\tau^{-1} \approx 1.5 \times 10^{-7} (GM/c^3)^{-1}, at Mμ0.42M \mu \approx 0.42. 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