Stochastic accretion impacts excite neutron star r-modes with root-mean-square GW strain near 1e-35 at 10 Hz, too weak for LIGO, plus an autocorrelation diagnostic for CFS instability.
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Gravitational waves from r-mode oscillations of stochastically accreting neutron stars
Stochastic accretion impacts excite neutron star r-modes with root-mean-square GW strain near 1e-35 at 10 Hz, too weak for LIGO, plus an autocorrelation diagnostic for CFS instability.