Extreme mass ratio inspirals: perspectives for their detection

Babak, Stanislav; Gair, Jonathan R.; Cole, Robert H.

doi:10.1007/978-3-319-18335-0_23

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Extreme mass ratio inspirals: perspectives for their detection

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Babak, Stanislav
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Zitation

Babak, S., Gair, J. R., & Cole, R. H. (2015). Extreme mass ratio inspirals: perspectives for their detection. In Equations of Motion in Relativistic Gravity. Fundamental Theories of Physics, 179 (pp. 783-812).

Zitierlink: https://hdl.handle.net/11858/00-001M-0000-002A-FC2C-9

Zusammenfassung

In this article we consider prospects for detecting extreme mass ratio inspirals (EMRIs) using gravitational wave (GW) observations by a future space borne interferometric observatory eLISA. We start with a description of EMRI formation channels. Different formation scenarios lead to variations in the expected event rate and predict different distributions of the orbital parameters when the GW signal enters the eLISA sensitivity band. Then we will briefly overview the available theoretical models describing the GW signal from EMRIs and describe proposed methods for their detection.