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Black Hole Solar Systems Extreme Mass Ratio InspiralsWaveforms known well enough to detect some EMRIs today. Soon, enough to realize Gair et al estimate of approx. 100's to 1000's of detections to z = 1. Not yet enough to for precision parameter estimation of Barack and Cutler (mass and spin to 10(exp -4)). Some turning to the more exotic: non-Kerr background, gas interaction, third body, ... More status and refs: Drasco, gr-qc/0604115.
Document ID
20060050277
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
hdl:2014/39707
Authors
Drasco, Steve (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 23, 2013
Publication Date
January 1, 2006
Subject Category
Astrophysics
Meeting Information
Meeting: Physics of Galactic Nuclei
Location: Santa Barbara, CA
Country: United States
Start Date: June 22, 2006
Distribution Limits
Public
Copyright
Other
Keywords
general relativity
Laser Interferometer Space Antenna (LISA)
gravity
Black Holes

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