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The capture and subsequent inspiral of stellar mass black holes on eccentricorbits by central massive black holes, is one of the more interesting likelysources of gravitational radiation detectable by LISA. We estimate the rate ofobservable events and the associated uncertainties. A moderately favourablemass function could provide many detectable bursts each year, and a detectionof at least one burst per year is very likely given our current understandingof the populations in cores of normal spiral galaxies.Comment: 3 pages 2-column revtex Latex macro. No figures. Classical and  Quantum Gravity, accepte

Estimating the detectable rate of capture of stellar mass black holes by massive central black holes in normal galaxies