Compact Binary Coalescence
Compact Binary Coalescence is a dynamical astrophysical process, within the framework of general relativity and the post-Newtonian approximation, in which two compact objects—such as neutron stars or black holes—lose orbital energy through gravitational wave emission, inspiral, and ultimately merge into a single compact object.
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759
Institutions
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2017–2026
267
Variants
Cbc
494
GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
B. P. Abbott, R. Abbott, T. D. Abbott et al. · Physical Review Letters · 2017 · 2.5K citations · Full text
Natural Sciences, Astronomy, Physics +13
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California Institute of Technology
Pasadena, United States
63 h-index
3.4K publications
1.3M citations
Max Planck Institute for Gravitational Physics
Potsdam, Germany
52 h-index
2.9K publications
1.2M citations
Cardiff University
Cardiff, United Kingdom
50 h-index
878 publications
376K citations

University of Birmingham
Birmingham, United Kingdom
49 h-index
783 publications
341.2K citations
Massachusetts Institute of Technology
Cambridge, United States
47 h-index
1.4K publications
619.3K citations
Northwestern University
Evanston, United States
46 h-index
454 publications
181.4K citations

University of Wisconsin–Milwaukee
Milwaukee, United States
46 h-index
883 publications
349.9K citations
University of Maryland, College Park
College Park, United States
46 h-index
223 publications
69.9K citations
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PRD · 121 publications · 8.7K citations
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ApJ · 65 publications · 9K citations
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53 publications · 6.7K citations
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