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Fig. C.1.

image

Fraction of asteroids reaching the Roche limit via the quadrupolar Kozai-Lidov effect in the classical calculation (blue) and in the general relativity case (orange), as a function of the outer body inclination i2. Its mass is set to m1 = 10 M. The density of the asteroids are set to ρast = 2 g cm−3 and their semi-major axes follow a Normal law with mean semi-major axis ⟨aast⟩ = 1 AU and standard deviation σa = 0.15 ⟨aast⟩.

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