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The future detection of gravitational wave forces us to consider the manyways in which astrophysics, gravitational wave theory and fundamental theorywill interact. In this paper, I summarize some recent work done to develop suchan interface. In particular, I concentrate on how non-vacuum astrophysicalenvironments can modify the gravitational wave signal emitted by compact binaryinspirals, and whether signatures from the former are detectable by current andfuture gravitational wave detectors. I also describe the interface betweengravitational wave modeling and fundamental theory, focusing on the status ofthe parameterized post-Einsteinian framework (a general framework to detectdeviations away from General Relativity in future gravitational wave data) andits current data analysis implementation.

Gravitational Waves from Compact Binaries as Probes of the Universe