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Fig. 6.

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Evolution of key quantities relevant for the binary orbit after the initial envelope spin-up and adjustment. Panel a: moving average of the specific angular momentum transfer ⟨jP (Eq. (32)) for models A, B, C, and D. The black dashed line indicates the critical specific angular momentum transfer jcrit = 3/8. Panel b: moving average of the gravitational torque for simulation runs A and A′. The black dashed line indicates . Panel c: moving average of the mass accretion rate through the inner boundary ⟨P. Panel d: envelope mass in our numerical domain Menv(r ≤ 10). Panel e: moving average of the orbital separation evolution timescale .

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