A two-star extension of the earlier compact-component tidal theory shows that near critical curves with zero time-averaged apsidal precession, the apsidal angle librates and spin-orbit inclinations can undergo significant oscillations.
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On the non-dissipative orbital evolution of a binary system comprising non-compact components with misaligned spin and orbital angular momenta
A two-star extension of the earlier compact-component tidal theory shows that near critical curves with zero time-averaged apsidal precession, the apsidal angle librates and spin-orbit inclinations can undergo significant oscillations.