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...
Main Authors: | Tiwari, V., Klimenko, S., Christensen, N., Huerta, E. A., Gopakumar, A., Haney, M., Ajith, P., McWilliams, S. T., Vedovato, G., Drago, M., Salemi, F., Prodi, G. A., Lazzaro, C., Tiwari, S., Mitselmakher, G., Da Silva, F., Ray Pitambar Mohapatra, Satyanarayan |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research |
Format: | Article |
Language: | English |
Published: |
American Physical Society
2016
|
Online Access: | http://hdl.handle.net/1721.1/101152 |
Similar Items
-
Sensitivity comparison of searches for binary black hole coalescences with ground-based gravitational-wave detectors
by: Mohapatra, Satya, et al.
Published: (2014) -
LOCALIZATION OF SHORT DURATION GRAVITATIONAL-WAVE TRANSIENTS WITH THE EARLY ADVANCED LIGO AND VIRGO DETECTORS
by: Essick, Reed Clasey, et al.
Published: (2015) -
Highly eccentric inspirals into a black hole
by: Osburn, Thomas, et al.
Published: (2016) -
Constraining black hole mimickers with gravitational wave observations
by: Johnson-McDaniel, Nathan K, et al.
Published: (2022) -
Observation of Gravitational Waves from a Binary Black Hole Merger
by: Abbott, B. P., et al.
Published: (2016)