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We study analytically the Klein-Gordon wave equation for stationary massive scalar fields linearly coupled to spinning Kerr black holes.
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2010
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2010
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We shall use natural units in which G = c = ℏ = 1 G=c=\hbar=1
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Note that the proper mass μ \mu , which characterizes the scalar field mode, stands for μ / ℏ \mu/\hbar . Hence, this physical parameter of the matter field has the dimensions of ( ( length OPEN ) − 1 )^{-1}
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Here the dimensionless integer parameters m m and n n are respectively the azimuthal harmonic index and the resonance parameter of the stationary bound-state massive scalar field mode [see Eqs. ( 8
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We shall assume a > 0 a>0 and m > 0 m>0 for the black-hole-field physical parameters without loss of generality
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2016
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2016
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