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Research Update on Extreme-Mass-Ratio Inspirals

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.

preprint2014arXivOpen access
Pau Amaro-SeoaneJonathan R. GairAdam PoundScott A. HughesCarlos F. Sopuerta
astro-ph.COastro-ph.GAgr-qc
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Pau Amaro-SeoaneJonathan R. GairAdam PoundScott A. HughesCarlos F. Sopuerta

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