Characterize the accessibility of minidisk spin states
Characterize the conditions under which the retrograde circumbinary-binary system realizes the both-retrograde, both-prograde, or mixed minidisk spin states, and determine whether the both-prograde and both-retrograde states are equally accessible or whether one is preferred under realistic astrophysical conditions.
References
The initial conditions of the disk are the primary factor determining which spin state is realised, although we have not explored this systematically. The mixed $\uparrow\downarrow$ state also remains uncharacterised, due to the computational demands of eccentricity sweeps at Mach 40. Fully mapping the conditions under which each state is common (and the associated orbital evolution) is one of the most astrophysically relevant questions arising from this work. Dedicated simulations spanning a range of mass ratios, Mach numbers, and initial disk conditions would clarify whether the $\uparrow\uparrow$ and $\downarrow\downarrow$ states are equally accessible, or whether one is preferred under realistic astrophysical conditions.