Positive values of the SdS parameter accelerate eccentricity decay, shorten plunge times, and produce increased amplitude with cumulative phase advance in adiabatic waveforms for extreme-mass ratio inspirals.
Poisson, Metric of a tidally distorted nonrotating black hole, Physical review letters94, 161103 (2005)
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Extreme-mass ratio inspirals in Schwarzschild - de Sitter spacetime I: Weak-field orbits
Positive values of the SdS parameter accelerate eccentricity decay, shorten plunge times, and produce increased amplitude with cumulative phase advance in adiabatic waveforms for extreme-mass ratio inspirals.