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Table 2

Collected efficiency expressions used in recent studies.

Limit 2D/shear 3D i = e∕2 ≫ hP
Leading term ε qpηhP qpηiP
This work/Paper I 0.23 0.39 0.31
Chambers (2014)a 0.31 0.5 0.5
Morbidelli et al. (2015)b 0.36 0.33c
Ida et al. (2016)d 0.46 0.40

Notes. In comparing the expressions we adopt the shear-dominated velocity regime in the 2D limit (massive planets). (a) Using their Eqs. (1), (29) and (31). (b)In the 2D limitthe expression followed Lambrechts & Johansen (2014). Bitsch et al. (2015) also adopts these expressions. (c) Did not obtain the correct leading term in the case when the approach velocity was given by the Keplerian shear. (d) Their Eq. (59).

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