A matrix-based extension of Papaloizou (2015) gives the tidal separation timescale T for N-planet chains and converts observed offsets into effective Q' bounds, with special sensitivity to the second and outermost planet masses.
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Two-fluid model shows black holes persist through cosmological bounce and modify background fluid properties under fixed geometry.
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How to measure tidal dissipation in long resonant chains
A matrix-based extension of Papaloizou (2015) gives the tidal separation timescale T for N-planet chains and converts observed offsets into effective Q' bounds, with special sensitivity to the second and outermost planet masses.
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Black holes in a bouncing universe
Two-fluid model shows black holes persist through cosmological bounce and modify background fluid properties under fixed geometry.