Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during Their First and Second Observing Runs

Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during Their First and Second Observing Runs

© 2019. The American Astronomical Society. When formed through dynamical interactions, stellar-mass binary black holes (BBHs) may retain eccentric orbits (e > 0.1 at 10 Hz) detectable by ground-based gravitational-wave detectors. Eccentricity can therefore be used to differentiate dynamically for...

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Bibliographic Details
Main Authors: LIGO Scientific Collaboration, Virgo Collaboration, Aggarwal, Nancy, Barnum, Sam, Barsotti, Lisa, Biscans, Sebastien, Biscoveanu, Sylvia, Buikema, Aaron, Demos, Nicholas, Donovan, Frederick J, Eisenstein, Robert Alan, Evans, Matthew J, Fernandez Galiana, Alvaro-Miguel, Fishner, Jason M., Fritschel, Peter K, Gras, Slawomir, Hall, E. D., Haster, Carl-Johan, Huang, Y., Isi Banales, Maximiliano S, Katsavounidis, Erotokritos, Lane, B. B., Lanza Jr, Robert K, London, L. T., Lynch, Ryan Christopher, MacInnis, Myron E, Mansell, Georgia, Mason, Kenneth R, Matichard, Fabrice, Mavalvala, Nergis, McCuller, Lee P, Mittleman, Richard K, Ray Pitambar Mohapatra, Satyanarayan, Ng, Kwan Yeung, Shoemaker, David H, Sudhir, Vivishek, Tse, Maggie, Vitale, Salvatore, Weiss, Rainer, Whittle, Christopher Mark, Yu, Hang, Yu, Haocun, Zucker, Michael E
Other Authors: LIGO (Observatory : Massachusetts Institute of Technology)
Format: Article
Language:English
Published: American Astronomical Society 2022
Online Access:https://hdl.handle.net/1721.1/132414.2

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https://hdl.handle.net/1721.1/132414.2

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