Abstract
Ultracompact binaries are expected to be the best candidates for continuous gravitational radiation in the frequency range of space-based gravity wave detectors such as LISA. The dynamics of globular cluster evolution are expected to enhance the population of such binaries in globular clusters. We present the nature of the globular cluster population of binaries which will be detectable by LISA as well as the fraction of the galactic globular cluster system which can be explored by LISA.
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