Proposed search for the detection of gravitational waves from eccentric binary black holes

Proposed search for the detection of gravitational waves from eccentric binary black holes

Most compact binary systems are expected to circularize before the frequency of emitted gravitational waves (GWs) enters the sensitivity band of the ground based interferometric detectors. However, several mechanisms have been proposed for the formation of binary systems, which retain eccentricity t...

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Main Authors: Tiwari, V. (Author), Klimenko, S. (Author), Christensen, N. (Author), Huerta, E. A (Author), Gopakumar, A. (Author), Haney, M. (Author), Ajith, P. (Author), McWilliams, S. T (Author), Vedovato, G. (Author), Drago, M. (Author), Salemi, F. (Author), Prodi, G. A (Author), Lazzaro, C. (Author), Tiwari, S. (Author), Mitselmakher, G. (Author), Da Silva, F. (Author), Ray Pitambar Mohapatra, Satyanarayan (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor), Mohapatra, Satya (Contributor)
Format: Article
Language:English
Published: American Physical Society, 2016-02-11T01:03:35Z.
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