Fig. 2
a) Dependence of the capture cross-section σ on DMP energy w for Sun-Jupiter (black curve, data from Ref. (8)) and for the Kepler map at J = 0.005 (red curve); the dashed line shows the dependence σ ∝ 1/|w |. b) Dependence of the rescaled captured number of DMPs on energy w for the models of the left panel. Here wcap = 0.001.
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