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Emergent flux from particle collisions near a Kerr black hole

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FIG. 1 (color online). A plot of turning points for Schwarzschild black holes in terms of b as a function of r (in units where R s ¼ 1)
FIG. 2 (color online). Escape fraction for a massless particle in the gravitational field of a Schwarzschild black hole as a function of r for DM particles colliding with angular momentum 	 1 ¼ 2 and 	 2 ¼ 2.
FIG. 3 (color online). Plot of turning points for an extremal Kerr black hole in terms of b as a function of r
FIG. 5 (color online). The escape fraction versus CMF energy for two DM particles colliding with angular momentum 	 1 ¼ 2 and 	 1 ¼ 2 in the gravitational field of a Kerr black hole with a ¼ 1

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