Gravitational Waves from Compact Objects Accreting onto Active Galactic Nuclei

We consider a model in which massive stars form in a self-gravitating accretion disk around an active galactic nucleus. These stars may evolve and collapse to form compact objects on a time scale shorter than the accretion time, thus producing an important family of sources for LISA. Assuming the compact object formation/inspiral rate is proportional to the steady-state gas accretion rate, we use the observed extra-galactic X-ray luminosity function to estimate expected event rates and signal strengths. We find that these sources will produce a continuous low-frequency background detectable by LISA if more than ∼> 1% of the accreted matter is in the form of compact objects. For compact objects with m ∼> 10M⊙, the last stages of the inspiral events should be resolvable above a few mHz, at a rate of ∼ 10−100 per year.