Numerical simulations show the gravitational wave strain from a 1 solar mass unstable disc in a tidal disruption event is about 4e-24, two orders below analytic estimates, and only a speculative extrapolation to 10-100 solar mass discs may be detectable by LISA.
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Gravitational wave emission from unstable accretion discs in tidal disruption events
Numerical simulations show the gravitational wave strain from a 1 solar mass unstable disc in a tidal disruption event is about 4e-24, two orders below analytic estimates, and only a speculative extrapolation to 10-100 solar mass discs may be detectable by LISA.