Fig. 6
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Same as Fig. 1, but using embryos instead of a planetesimal disk. The blue and green plots show the geometrical mean of eccentricities and inclinations of embryos. The blue solid line shows Eq. (5) with ⟨e0⟩ = 1 × 10−3. The green solid and dashed lines show Eq. (14) with ⟨sin i0⟩ = 5 × 10−4 and ⟨sin i0⟩ = hemb, respectively. Here, we show the results of 1 M⊕ embryos around 0.4 au.
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