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Research Update on Extreme-Mass-Ratio Inspirals

2014/10/03 by Pau Amaro-Seoane, Jonathan R. Gair, Adam Pound +2 · 1 citation
Physics and Astronomy · #astro-ph.CO #astro-ph.GA #gr-qc

paper · pdf · doi:10.1088/1742-6596/610/1/012002

17 pages, no figures. Proceedings of the LISA Symposium X, to be published at the Journal of Physics

arxiv created 2014/10/03 · arxiv updated 2015/06/11

Abstract

The inspirals of stellar-mass mass compact objects into massive black holes in the centres of galaxies are one of the most important sources of gravitational radiation for space-based detectors like LISA or eLISA. These extreme-mass-ratio inspirals (EMRIs) will enable an ambitious research program with implications for astrophysics, cosmology, and fundamental physics. This article is a summary of the talks delivered at the plenary session on EMRIs at the 10th International LISA Symposium. It contains research updates on the following topics: astrophysics of EMRIs; EMRI science potential; and EMRI modeling.

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