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...

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Main Authors: Amaro-Seoane, Pau, Gair, Jonathan R, Pound, Adam, Hughes, Scott A, Sopuerta, Carlos F
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: IOP Publishing 2017
Online Access:http://hdl.handle.net/1721.1/108542
https://orcid.org/0000-0001-6211-1388
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author Amaro-Seoane, Pau
Gair, Jonathan R
Pound, Adam
Hughes, Scott A
Sopuerta, Carlos F
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Amaro-Seoane, Pau
Gair, Jonathan R
Pound, Adam
Hughes, Scott A
Sopuerta, Carlos F
author_sort Amaro-Seoane, Pau
collection MIT
description 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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spelling mit-1721.1/1085422022-09-30T22:44:10Z Research Update on Extreme-Mass-Ratio Inspirals Amaro-Seoane, Pau Gair, Jonathan R Pound, Adam Hughes, Scott A Sopuerta, Carlos F Massachusetts Institute of Technology. Department of Physics MIT Kavli Institute for Astrophysics and Space Research Hughes, Scott A 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. National Science Foundation (U.S.) (PHY-1403261) 2017-05-01T18:06:21Z 2017-05-01T18:06:21Z 2015-05 2015-04 Article http://purl.org/eprint/type/JournalArticle 1742-6588 1742-6596 http://hdl.handle.net/1721.1/108542 Amaro-Seoane, Pau; Gair, Jonathan R; Pound, Adam; Hughes, Scott A and Sopuerta, Carlos F. “Research Update on Extreme-Mass-Ratio Inspirals.” Journal of Physics: Conference Series 610 (May 2015): 012002. © Copyright 2015 IOP Publishing https://orcid.org/0000-0001-6211-1388 en_US http://dx.doi.org/10.1088/1742-6596/610/1/012002 Journal of Physics: Conference Series Creative Commons Attribution 3.0 Unported license http://creativecommons.org/licenses/by/3.0/ application/pdf IOP Publishing IOP Publishing
spellingShingle Amaro-Seoane, Pau
Gair, Jonathan R
Pound, Adam
Hughes, Scott A
Sopuerta, Carlos F
Research Update on Extreme-Mass-Ratio Inspirals
title Research Update on Extreme-Mass-Ratio Inspirals
title_full Research Update on Extreme-Mass-Ratio Inspirals
title_fullStr Research Update on Extreme-Mass-Ratio Inspirals
title_full_unstemmed Research Update on Extreme-Mass-Ratio Inspirals
title_short Research Update on Extreme-Mass-Ratio Inspirals
title_sort research update on extreme mass ratio inspirals
url http://hdl.handle.net/1721.1/108542
https://orcid.org/0000-0001-6211-1388
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