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  Extreme mass ratio inspirals: perspectives for their detection

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).

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-002A-FC2C-9 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-002C-412D-B
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 Creators:
Babak, Stanislav1, Author           
Gair, Jonathan R., Author
Cole, Robert H., Author
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc,Astrophysics, Cosmology and Extragalactic Astrophysics, astro-ph.CO
 Abstract: 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.

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 Dates: 2014-11-192015
 Publication Status: Issued
 Pages: 39 pages, 4 figures, to appear in proceedings of EOM 2013 "Equations of Motion in Relativistic Gravity"
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 Identifiers: arXiv: 1411.5253
URI: http://arxiv.org/abs/1411.5253
DOI: 10.1007/978-3-319-18335-0_23
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Title: Equations of Motion in Relativistic Gravity. Fundamental Theories of Physics, 179
Source Genre: Book
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Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 783 - 812 Identifier: -