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The massive Galactic black hole and the stars around it are a uniquelaboratory for studying how relaxation processes lead to close interactions ofstars and compact remnants with the central massive black hole, in particularthose leading to the emission of gravitational waves. I review new results onthe processes of strong mass segregation and loss-cone refilling by massiveperturbers and resonant relaxation; describe observational evidence that theseprocesses play a role in the Galactic Center and can be studied there; anddiscuss some of the implications for Extreme Mass Ration Inspiral event ratesand their properties.

The Galactic Center as a laboratory for extreme mass ratio gravitational wave source dynamics