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The unique potential of extreme mass-ratio inspirals for gravitational-wave astronomy

Published onMay 31, 2019
The unique potential of extreme mass-ratio inspirals for gravitational-wave astronomy
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Abstract

EMRIs are a prime source for LISA. They will tell us about the stellar dynamics in galactic nuclei and massive black hole populations. They will enable percent-level measurements of the multipolar structure of massive black holes and tests of the strong-gravity regime. They may also provide cosmographical data about the expansion of the Universe.

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